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1. Modeling of 35-day superorbital cycle of $B$ and $V$ light curves of IMXB HZ Her/Her X-1

Author

Kolesnikov, D. A., Shakura, N. I., Postnov, K. A., Volkov, I. M., Bikmaev, I. F., Irsmambetova, T. R., Staubert, R., Wilms, J., Irtuganov, E., Golyshev, P. Yu., Shugarov, S. Yu., Nikolenko, I. V., Trunkovsky, E. M., Schönherr, G., Schwope, A., and Klochkov, D.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The X-ray binary Her X-1 consists of an accreting neutron star and the optical component HZ Her. The 35-day X-ray superorbital variability of this system is known since its discovery in 1972 by the Uhuru satellite and is believed to be caused by forced precession of a warped accretion disk tilted to the orbital plane. We argue that the observed features of the 35-day optical variability of HZ Her can be explained by free precession of the neutron star with a period close to that of the forced disk. The model parameters include a) the X-ray luminosity of the neutron star; b) the optical flux from the accretion disk; c) the tilt of the inner and outer edges of the accretion disk. A possible synchronization mechanism based on the coupling between the neutron star free precession and the dynamical action of non-stationary gas streams is discussed., Comment: 12 pages, 11 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society Main Journal

Published
2020
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2. Rapid quasi-periodic oscillations in the relativistic jet of BL Lacertae

Author

Jorstad, S. G., Marscher, A. P., Raiteri, C. M., Villata, M., Weaver, Z. R., Zhang, H., Dong, L., Gómez, J. L., Perel, M. V., Savchenko, S. S., Larionov, V. M., Carosati, D., Chen, W. P., Kurtanidze, O. M., Marchini, A., Matsumoto, K., Mortari, F., Aceti, P., Acosta-Pulido, J. A., Andreeva, T., Apolonio, G., Arena, C., Arkharov, A., Bachev, R., Banfi, M., Bonnoli, G., Borman, G. A., Bozhilov, V., Carnerero, M. I., Damljanovic, G., Ehgamberdiev, S. A., Elsässer, D., Frasca, A., Gabellini, D., Grishina, T. S., Gupta, A. C., Hagen-Thorn, V. A., Hallum, M. K., Hart, M., Hasuda, K., Hemrich, F., Hsiao, H. Y., Ibryamov, S., Irsmambetova, T. R., Ivanov, D. V., Joner, M. D., Kimeridze, G. N., Klimanov, S. A., Knött, J., Kopatskaya, E. N., Kurtanidze, S. O., Kurtenkov, A., Kuutma, T., Larionova, E. G., Leonini, S., Lin, H. C., Lorey, C., Mannheim, K., Marino, G., Minev, M., Mirzaqulov, D. O., Morozova, D. A., Nikiforova, A. A., Nikolashvili, M. G., Ovcharov, E., Papini, R., Pursimo, T., Rahimov, I., Reinhart, D., Sakamoto, T., Salvaggio, F., Semkov, E., Shakhovskoy, D. N., Sigua, L. A., Steineke, R., Stojanovic, M., Strigachev, A., Troitskaya, Y. V., Troitskiy, I. S., Tsai, A., Valcheva, A., Vasilyev, A. A., Vince, O., Waller, L., Zaharieva, E., and Chatterjee, R.

Published
2022
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3. Dynamics of wind and the dusty environments in the accreting T Tauri stars RY Tau and SU Aur

Author

Petrov, P. P., Grankin, K. N., Gameiro, J. F., Artemenko, S. A., Babina, E. V., de Albuquerque, R. M. G., Djupvik, A. A., Gahm, G. F., Shenavrin, V. I., Irsmambetova, T. R., Fernandez, M., Mkrtichian, D. E., and Gorda, S. Yu.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

Classical T Tauri stars with ages of less than 10 Myr possess accretion discs. Magnetohydrodynamic processes at the boundary between the disc and the stellar magnetosphere control the accretion and ejections gas flows. We carried out a long series of simultaneous spectroscopic and photometric observations of the classical T Tauri stars RY Tau and SU Aur with the aim to quantify the accretion and outflow dynamics at time scales from days to years. It is shown that dust in the disc wind is the main source of photometric variability of these stars. In RY Tau we observed a new effect: during events of enhanced outflow the circumstellar extinction gets lower. The characteristic time of changes in outflow velocity and stellar brightness indicates that the obscuring dust is near the star. The outflow activity in both stars is changing on a time scale of years. Periods of quiescence in H$\alpha$ profile variability were observed during 2015-2016 season in RY Tau and during 2016-2017 season in SU Aur. We interpret these findings in the framework of the magnetospheric accretion model, and discuss how the global stellar magnetic field may influence the long-term variations of the outflow activity., Comment: 17 pages, 13 figures, 4 tables, accepted for publication in MNRAS

Published
2018
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4. SU Aur: A Deep Fading Event in Visible and Near-Infrared Bands

Author

Grankin, K. N., Shenavrin, V. I., Irsmambetova, T. R., and Petrov, P. P.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

In three seasons of 2015-2018 we carried out a series of visible and near infrared (NIR) photometry of SU Aur. In course of this photometric monitoring we detected an event of a deep fading of the star in spring of 2018. In this paper we present preliminary analysis of our photometry., Comment: 4 pages, 2 figures

Published
2018
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6. Timing of AB And eclipses

Author

Kozyreva, V. S., Ibrahimov, M. A., Gaynullina, E. R., Karimov, R. G., Hafizov, B. M., Satovskii, B. L., Krushevska, V. N., Kuznyetsova, Yu. G., Bogomazov, A. I., Irsmambetova, T. R., and Tutukov, A. V.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

This study aims timing the eclipses of the short period low mass binary star AB And. The times of minima are taken from the literature and from our observations in October 2013 (22 times of minima) and in August 2014 (23 times of minima). We find and discuss an inaccuracy in the determination of the types of minima in the previous investigation by \citet{li2014}. We study the secular evolution of the central binary's orbital period and the possibility of the existence of third and fourth companions in the system., Comment: 14 pages, 3 figures, 3 tables, accepted by New Astronomy

Published
2017
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7. Light equation in eclipsing binary CV Boo: third body candidate in elliptical orbit

Author

Bogomazov, A. I., Kozyreva, V. S., Satovskii, B. L., Krushevska, V. N., Kuznyetsova, Yu. G., Ehgamberdiev, Sh. A., Karimov, R. G., Khalikova, A. V., Ibrahimov, M. A., Irsmambetova, T. R., and Tutukov, A. V.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

A short period eclipsing binary star CV Boo is tested for the possible existence of additional bodies in the system with a help of the light equation method. We use data on the moments of minima from the literature as well as from our observations during 2014 May--July. A variation of the CV Boo's orbital period is found with a period of $\approx 75$ d. This variation can be explained by the influence of a third star with a mass of $\approx 0.4M_{\odot}$ in an eccentric orbit with $e\approx 0.9$. A possibility that the orbital period changes on long time scales is discussed. The suggested tertiary companion is near the chaotic zone around the central binary, so CV Boo represents an interesting example to test its dynamical evolution. A list of 14 minima moments of the binary obtained from our observations is presented., Comment: 8 pages, 4 figures, 1 table, accepted for publication in Ap&SS

Published
2016
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8. Timing of eclipsing binary V0873 Per: a third body candidate

Author

Bogomazov, A. I., Ibrahimov, M. A., Satovsky, B. L., Kozyreva, V. S., Irsmambetova, T. R., Krushevska, V. N., Kuznyetsova, Yu. G., Gaynullina, E. R., Karimov, R. G., Ehgamberdiev, Sh. A., and Tutukov, A. V.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We analyse a set of moments of minima of eclipsing variable V0873 Per. V0873 Per is a short period low mass binary star. Data about moments of minima of V0873 Per were taken from literature and our observations during 2013-2014. Our aim is to test the system on existence of new bodies using timing of minima of eclipses. We found the periodical variation of orbital period of V0873 Per. This variation can be explained by the gravitational influence of a third companion on the central binary star. The mass of third body candidate is $\approx 0.2 M_{\odot}$, its orbital period is $\approx 300$ days. The paper also includes a table with moments of minima calculated from our observations which can be used in future investigations of V0873 Per., Comment: 8 pages, 5 figures, 4 tables, accepted for publication in Astrophysics and Space Science

Published
2015
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9. INTEGRAL observations of SS433: Results of coordinated campaign

Author

Cherepashchuk, A. M., Sunyaev, R. A., Fabrika, S. N., Postnov, K. A., Molkov, S. V., Barsukova, E. A., Antokhina, E. A., Irsmambetova, T. R., Panchenko, I. E., Seifina, E. V., Shakura, N. I., Timokhin, A. N., Bikmaev, I. F., Sakhibullin, N. A., Aslan, Z., Khamitov, I., Pramsky, A. G., Sholukhova, O., Gnedin, Yu. N., Arkharov, A. A., and Larionov, V. M.

Subjects
Astrophysics
Abstract

Results of simultaneous INTEGRAL and optical observations of galactic microquasar SS433 in May 2003 and INTEGRAL/RXTE observations in March 2004 are presented. Persistent precessional variability with a maximum to minimum uneclipsed hard X-ray flux ratio of \sim 4 is discovered. The 18-60 keV X-ray eclipse is found to be in phase with optical and near infrared eclipses. The orbital eclipse observed by INTEGRAL in May 2003 is at least two times deeper and apparently wider than in soft X-ray band. The broadband X-ray spectrum 2-100 keV simultaneously detected by RXTE/INTEGRAL in March 2004 can be described by bremsstrahlung emission from optically thin thermal plasma with kT\sim 30 keV. The optical spectroscopy with the 6-m SAO BTA telescope confirmed the optical companion to be an A5-A7 supergiant. For the first time, spectorscopic indications of a strong heating effect in the optical star atmosphere are found. The measurements of absorption lines which are presumably formed in the non-illuminated side of the supergiant yield its radial velocity semi-amplitude K_v=132\pm 9 km/s. The analysis of the observed hard X-ray light curve and the eclipse duration, combined with spectroscopically found optical star radial velocity corrected for the strong heating effect, allows us to model SS433 as a massive X-ray binary. Assuming that the hard X-ray source in SS433 is eclipsed by the donor star that exactly fills its Roche lobe, the masses of the optical and compact components in SS433 are suggested to be M_v\approx 30 M_\odot and M_x\approx 9M_\odot, respectively. This provides further evidence that SS433 is a massive binary system with supercritical accretion onto a black hole., Comment: 15 pages, AA style, 17 figures, accepted for publication in AA; replaced to match the accepted version

Published
2005
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10. Coordinated INTEGRAL and optical observations of SS433

Author

Cherepashchuk, A. M., Sunyaev, R. A., Fabrika, S. N., Molkov, S. V., Barsukova, E. A., Antokhina, E. A., Irsmambetova, T. R., Panchenko, I. E., Postnov, K. A., Seifina, E. V., Shakura, N. I., Timokhin, A. N., Bikmaev, I. F., Sakhibullin, N. A., Gnedin, Yu. N., Arkharov, A. A., and Larionov, V. M.

Subjects
Astrophysics
Abstract

Results of simultaneous {\it INTEGRAL} and optical observations of galactic microquasar SS433 in May 2003 are presented. The analysis of the X-ray and optical eclipse duration and hard X-ray spectra obtained by {\it INTEGRAL} together with optical spectroscopy obtained on the 6-m telescope allows us to construct a model of SS433 as a massive X-ray binary. X-ray eclipse in hard X-rays has a depth of $\sim 80%$ and extended wings. The optical spectroscopy allows us to identify the optical companion as a A5-A7 supergiant and to measure its radial velocity semi-amplitude $K_v=132$ km/s. A strong heating effect in the optical star atmosphere is discovered spectroscopically. The observed broadband X-ray spectrum 2-100 keV can be described by emission from optically thin thermal plasma with $kT\sim 15-20 keV$, Comment: 8 pages, 11 figures, Proceedings of the V INTEGRAL Workshop, Munich 16-20 February 2004. ESA SP-552

Published
2004

13. Astrometric results of observations at Russian observatories of mutual occultations and eclipses of Jupiter’s Galilean satellites in 2009

Author

Emelyanov, N. V., Andreev, M. V., Berezhnoi, A. A., Bekhteva, A. S., Vashkovyak, S. N., Velikodskii, Yu. I., Vereshchagina, I. A., Gorshanov, D. L., Devyatkin, A. V., Izmailov, I. S., Ivanov, A. V., Irsmambetova, T. R., Kozlov, V. A., Karashevich, S. V., Kurenya, A. N., Naiden, Ya. V., Naumov, K. N., Parakhin, N. A., Raskhozhev, V. N., Selyaev, S. A., Sergeev, A. V., Sokov, E. N., Khovrichev, M. Yu., Khrutskaya, E. V., and Chernikov, M. M.

Published
2011
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14. Modelling Of 35-D Superorbital Cycle Of B And V Light Curves Of Imxb Hz Her/Her X-1

Author

Kolesnikov, D. A., Shakura, N., I, Postnov, K. A., Volkov, I. M., Bikmaev, I. F., Irsmambetova, T. R., Staubert, R., Wilms, J., Irtuganov, E., Golysheva, P. Yu, Shugarov, S. Yu, Nikolenko, I., V, Trunkovsky, E. M., Schoenherr, G., Schwope, A., and Klochkov, D.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

The X-ray binary Her X-1 consists of an accreting neutron star and the optical component HZ Her. The 35-d X-ray superorbital variability of this system is known, since its discovery in 1972 by the Uhuru satellite and is believed to be caused by forced precession of a warped accretion disc tilted to the orbital plane. We argue that the observed features of the 35-d optical variability of HZ Her can be explained by free precession of the neutron star with a period close to that of the forced disc. The model parameters include (a) the X-ray luminosity of the neutron star; (b) the optical flux from the accretion disc; and (c) the tilt of the inner and outer edges of the accretion disc. A possible synchronization mechanism based on the coupling between the neutron star free precession and the dynamical action of non-stationary gas streams is discussed.

Published
2020

16. Modelling of 35-d superorbital cycle of B and V light curves of IMXB HZ Her/Her X-1

Author

Kolesnikov, D A, primary, Shakura, N I, additional, Postnov, K A, additional, Volkov, I M, additional, Bikmaev, I F, additional, Irsmambetova, T R, additional, Staubert, R, additional, Wilms, J, additional, Irtuganov, E, additional, Golysheva, P Yu, additional, Shugarov, S Yu, additional, Nikolenko, I V, additional, Trunkovsky, E M, additional, Schönherr, G, additional, Schwope, A, additional, and Klochkov, D, additional

Published
2020
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17. Progress in the Research of the Relativistic System SS 433

Author

Goranskij, V. P., primary, Barsukova, E. A., additional, Burenkov, A. N., additional, Valeev, A. F., additional, Volkov, \I. M., additional, Zubareva, A. M., additional, Esipov, V. F., additional, Ikonnikova, N. P., additional, Irsmambetova, T. R., additional, Pavlyuk, N. N., additional, and Shugarov, S. Yu., additional

Published
2020
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18. Dynamics of wind and the dusty environments in the accreting T Tauri stars RY Tauri and SU Aurigae

Author

Petrov, P. P., Grankin, K. N., Gameiro, J. F., Artemenko, S. A., Babina, E. V., De Albuquerque, R. M. G., Djupvik, A. A., Gahm, G. F., Shenavrin, V. I., Irsmambetova, T. R., Fernandez, M., Mkrtichian, D. E., Gorda, S. Yu., Petrov, P. P., Grankin, K. N., Gameiro, J. F., Artemenko, S. A., Babina, E. V., De Albuquerque, R. M. G., Djupvik, A. A., Gahm, G. F., Shenavrin, V. I., Irsmambetova, T. R., Fernandez, M., Mkrtichian, D. E., and Gorda, S. Yu.

Abstract

Classical T Tauri stars with ages of less than 10 Myr possess accretion discs. Magnetohydro-dynamic processes at the boundary between the disc and the stellar magnetosphere control the accretion and ejections gas flows. We carried out a long series of simultaneous spectroscopic and photometric observations of the classical T Tauri stars, RY Tauri and SU Aurigae, with the aim to quantify the accretion and outflow dynamics at time-scales from days to years. It is shown that dust in the disc wind is the main source of photometric variability of these stars. In RY Tau, we observed a new effect: during events of enhanced outflow, the circumstellar extinction becomes lower. The characteristic time of changes in outflow velocity and stellar brightness indicates that the obscuring dust is near the star. The outflow activity in both stars is changing on a time-scale of years. Periods of quiescence in the variability of the Hα profile were observed during the 2015-2016 period in RY Tau and during the 2016-2017 period in SU Aur. We interpret these findings in the framework of the magnetospheric accretion model, and we discuss how the global stellar magnetic field can influence the long-term variations of the outflow activity. © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Published
2019

19. Timing of AB And eclipses

Author

Kozyreva, V. S, Ibrahimov, M. A, Gaynullina, E. R, Karimov, R. G, Hafizov, B. M, Satovskii, B. L, Krushevska, V. N, Kuznyetsova, Yu. G, Bogomazov, A. I, Irsmambetova, T. R, and Tutukov, A. V

Published
2018
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20. Timing of AR CrB eclipses

Author

Kozyreva V. S., Irsmambetova T. R., Ibrahimov M. A., Krushevska V. N., Kuznyetsova Yu G., Khalikova A. V., Parmonov O. U., Karimov R. G., Bogomazov A. I., Satovskii B. L., and Tutukov A. V.

Subjects
Physics, Astronomy and Astrophysics, Astrophysics, Instrumentation
Published
2018
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21. Light equation on eclipsing binary CV Boo

Author

Bogomazov, A. I., Kozyreva, V. S., Satovskii, B. L., Krushevska, V. N., Kuznyetsova, Yu. G., Ehgamberdiev, Sh. A., Karimov, R. G., Khalikova, A. V., Ibrahimov, M. A., Irsmambetova, T. R., and Tutukov, A. V.

Abstract

Короткопериодическая затменная двойная звезда CV Boo изучена методом светового уравнения. Были использованы данные о моментах минимумов из литературы и из наших наблюдений в мае июле 2014 г. Была найдена периодическая вариация орбитального периода системы с периодом ≈ 75 дней. Эта вариация может быть объяснена гравитационным воздействием третьего тела с массой ≈ 0.4 M⊙ на вытянутой орбите с эксцентриситетом e ≈ 0.9. Также обсуждается возможность изменения орбитального периода на больших шкалах времени. Предлагаемое третье тело находится близко к хаотической зоне вокруг центральной двойной, поэтому оно может быть интересно для изучения его динамической эволюции. A short period eclipsing binary star CV Boo is tested for the possible existence of new bodies in the system with a help of the light equation method. We use data about moments of minima from the literature and our observations during May—July 2014. A periodical variation of CV Boo’s orbital period is found, the variation’s period is ≈ 75 days. This variation can be explained by the gravitational influence of a third star with a mass ≈ 0.4M⊙ in an eccentric orbit with e ≈ 0.9. A possibility for orbital period changes in long time scales is discussed. The suggested tertiary companion is near the chaotic zone around the central binary, so it is an interesting example to test its dynamical evolution.

Published
2018

22. Accretion processes in astrophysics

Author

Shakura, N I, primary, Kolesnikov, D A, additional, Postnov, K A, additional, Volkov, I M, additional, Bikmaev, I F, additional, Irsmambetova, T R, additional, Staubert, R, additional, Wilms, J, additional, Irtuganov, E, additional, Shurygin, P, additional, Golysheva, P Yu, additional, Shugarov, S Yu, additional, Nikolenko, I V, additional, Trunkovsky, E M, additional, Schoenherr, G, additional, Schwope, A, additional, and Klochkov, D, additional

Published
2019
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23. Световое уравнение в затменной двойной CV Boo

Author

Bogomazov, A. I., Kozyreva, V. S., Satovskii, B. L., Krushevska, V. N., Kuznyetsova, Yu. G., Ehgamberdiev, Sh. A., Karimov, R. G., Khalikova, A. V., Ibrahimov, M. A., Irsmambetova, T. R., Tutukov, A. V., Богомазов, А. И., Козырева, В. С., Сатовский, Б. Л., Крушевская, В. Н., Кузнецова, Ю. Г., Эгамбердиев, Ш. А., Каримов, Р. Г., Халикова, А. В., Ибрагимов, М. А., Ирсмамбетова, Т. Р., Тутуков, А. В., Bogomazov, A. I., Kozyreva, V. S., Satovskii, B. L., Krushevska, V. N., Kuznyetsova, Yu. G., Ehgamberdiev, Sh. A., Karimov, R. G., Khalikova, A. V., Ibrahimov, M. A., Irsmambetova, T. R., Tutukov, A. V., Богомазов, А. И., Козырева, В. С., Сатовский, Б. Л., Крушевская, В. Н., Кузнецова, Ю. Г., Эгамбердиев, Ш. А., Каримов, Р. Г., Халикова, А. В., Ибрагимов, М. А., Ирсмамбетова, Т. Р., and Тутуков, А. В.

Abstract

Короткопериодическая затменная двойная звезда CV Boo изучена методом светового уравнения. Были использованы данные о моментах минимумов из литературы и из наших наблюдений в мае июле 2014 г. Была найдена периодическая вариация орбитального периода системы с периодом ≈ 75 дней. Эта вариация может быть объяснена гравитационным воздействием третьего тела с массой ≈ 0.4 M⊙ на вытянутой орбите с эксцентриситетом e ≈ 0.9. Также обсуждается возможность изменения орбитального периода на больших шкалах времени. Предлагаемое третье тело находится близко к хаотической зоне вокруг центральной двойной, поэтому оно может быть интересно для изучения его динамической эволюции., A short period eclipsing binary star CV Boo is tested for the possible existence of new bodies in the system with a help of the light equation method. We use data about moments of minima from the literature and our observations during May—July 2014. A periodical variation of CV Boo’s orbital period is found, the variation’s period is ≈ 75 days. This variation can be explained by the gravitational influence of a third star with a mass ≈ 0.4M⊙ in an eccentric orbit with e ≈ 0.9. A possibility for orbital period changes in long time scales is discussed. The suggested tertiary companion is near the chaotic zone around the central binary, so it is an interesting example to test its dynamical evolution.

Published
2018

25. Rapid evolution of the relativistic jet system SS 433

Author

Goranskij, V. P., primary, Barsukova, E. A., additional, Burenkov, A. N., additional, Valeev, A. F., additional, Trushkin, S. A., additional, Volkov, I. M., additional, Esipov, V. F., additional, Irsmambetova, T. R., additional, and Zharova, A. V., additional

Published
2018
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26. Dynamics of wind and the dusty environments in the accreting T Tauri stars RY Tauri and SU Aurigae.

Author

Petrov, P P, Grankin, K N, Gameiro, J F, Artemenko, S A, Babina, E V, Albuquerque, R M G de, Djupvik, A A, Gahm, G F, Shenavrin, V I, Irsmambetova, T R, Fernandez, M, Mkrtichian, D E, and Gorda, S Yu

Subjects
STARS, GALAXIES, ACCRETION (Astrophysics), MAGNETOHYDRODYNAMICS, STELLAR magnetic fields, COSMIC magnetic fields
Abstract

Classical T Tauri stars with ages of less than 10 Myr possess accretion discs. Magnetohydrodynamic processes at the boundary between the disc and the stellar magnetosphere control the accretion and ejections gas flows. We carried out a long series of simultaneous spectroscopic and photometric observations of the classical T Tauri stars, RY Tauri and SU Aurigae, with the aim to quantify the accretion and outflow dynamics at time-scales from days to years. It is shown that dust in the disc wind is the main source of photometric variability of these stars. In RY Tau, we observed a new effect: during events of enhanced outflow, the circumstellar extinction becomes lower. The characteristic time of changes in outflow velocity and stellar brightness indicates that the obscuring dust is near the star. The outflow activity in both stars is changing on a time-scale of years. Periods of quiescence in the variability of the Hα profile were observed during the 2015–2016 period in RY Tau and during the 2016–2017 period in SU Aur. We interpret these findings in the framework of the magnetospheric accretion model, and we discuss how the global stellar magnetic field can influence the long-term variations of the outflow activity. [ABSTRACT FROM AUTHOR]

Published
2019
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28. Timing of eclipsing binary V0873 Per: a third body candidate

Author

Bogomazov, A. I., primary, Ibrahimov, M. A., additional, Satovskii, B. L., additional, Kozyreva, V. S., additional, Irsmambetova, T. R., additional, Krushevska, V. N., additional, Kuznyetsova, Y. G., additional, Gaynullina, E. R., additional, Karimov, R. G., additional, Ehgamberdiev, S. A., additional, and Tutukov, A. V., additional

Published
2015
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29. The PHEMU03 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter

Author

Arlot, J. -E., Thuillot, W., Ruatti, C., Ahmad, A., Amosse, A., Anbazhagan, P., Andreyev, M., Antov, A., Appakutty, M., Asher, D., Aubry, S., Baron, N., Bassiere, N., Berthe, M., Bogdanovski, R., Bosq, F., Bredner, E., Buettner, D., Buromsky, M., Cammarata, S., Casas, R., Chis, G. D., Christou, A. A., Coquerel, J. -P., Corlan, R., Cremaschini, C., Crussaire, D., Cuypers, J., Dennefeld, M., Descamps, P., Devyatkin, A., Dimitrov, D., Dorokhova, T. N., Dorokhov, N. I., Dourneau, G., Duenas, M., Dumitrescu, A., Emelianov, N., Ferrara, D., Fiel, D., Fienga, A., Flatres, T., Foglia, S., Garlitz, J., Gerbos, J., Gilbert, R., Goncalves, R. M. D., Gonzales, D., Gorda, S. Yu., Gorshanov, D. L., Hansen, M. W., Harrington, M., Irsmambetova, T. R., Ito, Y., Ivanova, V., Izmailov, I. S., Khovritchev, M. Yu., Khrutskaya, E. V., Kieken, J., Kiseleva, T. P., Kuppuswamy, K., Lainey, V., Lavayssiere, M., Lazzarotti, P., Le Campion, J. -F., Lellouch, E., Li, Z. L., Lo Savio, E., Lou, M., Magny, E., Manek, J., Marinello, W., Marino, G., McAuliffe, J. P., Michelli, M., Moldovan, D., Montagnac, S., Moorthy, V., Nickel, O., Nier, J. M., Noel, T., Noyelles, B., Oksanen, A., Parrat, D., Pauwels, T., Peng, Q. Y., Pizzetti, G., Priban, V., Ramachandran, B., Rambaux, N., Rapaport, M., Rapavy, P., Rau, G., Sacre, J. -J., Sada, P. V., Salvaggio, F., Sarlin, P., Sciuto, C., Selvakumar, G., Sergeyev, A., Sidorov, M., Sorescu, S., Spampinato, S. A., Stellmacher, I., Trunkovsky, E., Tejfel, V., Tudose, V., Turcu, V., Ugarte, I., Vantyghem, P., Vasundhara, R., Vaubaillon, J., Velu, C., Venkataramana, A. K., Vidal-Sainz, J., Vienne, A., Vilar, J., Vingerhoets, P., Vollman, W., Arlot, J. -E., Thuillot, W., Ruatti, C., Ahmad, A., Amosse, A., Anbazhagan, P., Andreyev, M., Antov, A., Appakutty, M., Asher, D., Aubry, S., Baron, N., Bassiere, N., Berthe, M., Bogdanovski, R., Bosq, F., Bredner, E., Buettner, D., Buromsky, M., Cammarata, S., Casas, R., Chis, G. D., Christou, A. A., Coquerel, J. -P., Corlan, R., Cremaschini, C., Crussaire, D., Cuypers, J., Dennefeld, M., Descamps, P., Devyatkin, A., Dimitrov, D., Dorokhova, T. N., Dorokhov, N. I., Dourneau, G., Duenas, M., Dumitrescu, A., Emelianov, N., Ferrara, D., Fiel, D., Fienga, A., Flatres, T., Foglia, S., Garlitz, J., Gerbos, J., Gilbert, R., Goncalves, R. M. D., Gonzales, D., Gorda, S. Yu., Gorshanov, D. L., Hansen, M. W., Harrington, M., Irsmambetova, T. R., Ito, Y., Ivanova, V., Izmailov, I. S., Khovritchev, M. Yu., Khrutskaya, E. V., Kieken, J., Kiseleva, T. P., Kuppuswamy, K., Lainey, V., Lavayssiere, M., Lazzarotti, P., Le Campion, J. -F., Lellouch, E., Li, Z. L., Lo Savio, E., Lou, M., Magny, E., Manek, J., Marinello, W., Marino, G., McAuliffe, J. P., Michelli, M., Moldovan, D., Montagnac, S., Moorthy, V., Nickel, O., Nier, J. M., Noel, T., Noyelles, B., Oksanen, A., Parrat, D., Pauwels, T., Peng, Q. Y., Pizzetti, G., Priban, V., Ramachandran, B., Rambaux, N., Rapaport, M., Rapavy, P., Rau, G., Sacre, J. -J., Sada, P. V., Salvaggio, F., Sarlin, P., Sciuto, C., Selvakumar, G., Sergeyev, A., Sidorov, M., Sorescu, S., Spampinato, S. A., Stellmacher, I., Trunkovsky, E., Tejfel, V., Tudose, V., Turcu, V., Ugarte, I., Vantyghem, P., Vasundhara, R., Vaubaillon, J., Velu, C., Venkataramana, A. K., Vidal-Sainz, J., Vienne, A., Vilar, J., Vingerhoets, P., and Vollman, W.

Published
2009

30. The PHEMU03 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter

Author

Arlot, J.-E., primary, Thuillot, W., additional, Ruatti, C., additional, Ahmad, A., additional, Amossé, A., additional, Anbazhagan, P., additional, Andreyev, M., additional, Antov, A., additional, Appakutty, M., additional, Asher, D., additional, Aubry, S., additional, Baron, N., additional, Bassiere, N., additional, Berthe, M., additional, Bogdanovski, R., additional, Bosq, F., additional, Bredner, E., additional, Buettner, D., additional, Buromsky, M., additional, Cammarata, S., additional, Casas, R., additional, Chis, G. D., additional, Christou, A. A., additional, Coquerel, J.-P., additional, Corlan, R., additional, Cremaschini, C., additional, Crussaire, D., additional, Cuypers, J., additional, Dennefeld, M., additional, Descamps, P., additional, Devyatkin, A., additional, Dimitrov, D., additional, Dorokhova, T. N., additional, Dorokhov, N. I., additional, Dourneau, G., additional, Dueñas, M., additional, Dumitrescu, A., additional, Emelianov, N., additional, Ferrara, D., additional, Fiel, D., additional, Fienga, A., additional, Flatres, T., additional, Foglia, S., additional, Garlitz, J., additional, Gerbos, J., additional, Gilbert, R., additional, Goncalves, R. M. D., additional, Gonzãles, D., additional, Gorda, S. Yu., additional, Gorshanov, D. L., additional, Hansen, M. W., additional, Harrington, M., additional, Irsmambetova, T. R., additional, Ito, Y., additional, Ivanova, V., additional, Izmailov, I. S., additional, Khovritchev, M. Yu., additional, Khrutskaya, E. V., additional, Kieken, J., additional, Kiseleva, T. P., additional, Kuppuswamy, K., additional, Lainey, V., additional, Lavayssiére, M., additional, Lazzarotti, P., additional, Le Campion, J.-F., additional, Lellouch, E., additional, Li, Z. L., additional, Lo Savio, E., additional, Lou, M., additional, Magny, E., additional, Manek, J., additional, Marinello, W., additional, Marino, G., additional, McAuliffe, J. P., additional, Michelli, M., additional, Moldovan, D., additional, Montagnac, S., additional, Moorthy, V., additional, Nickel, O., additional, Nier, J. M., additional, Noel, T., additional, Noyelles, B., additional, Oksanen, A., additional, Parrat, D., additional, Pauwels, T., additional, Peng, Q. Y., additional, Pizzetti, G., additional, Priban, V., additional, Ramachandran, B., additional, Rambaux, N., additional, Rapaport, M., additional, Rapavy, P., additional, Rau, G., additional, Sacré, J.-J., additional, Sada, P. V., additional, Salvaggio, F., additional, Sarlin, P., additional, Sciuto, C., additional, Selvakumar, G., additional, Sergeyev, A., additional, Sidorov, M., additional, Sorescu, S., additional, Spampinato, S. A., additional, Stellmacher, I., additional, Trunkovsky, E., additional, Tejfel, V., additional, Tudose, V., additional, Turcu, V., additional, Ugarte, I., additional, Vantyghem, P., additional, Vasundhara, R., additional, Vaubaillon, J., additional, Velu, C., additional, Venkataramana, A. K., additional, Vidal-Sãinz, J., additional, Vienne, A., additional, Vilar, J., additional, Vingerhoets, P., additional, and Vollman, W., additional

Published
2008
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32. The PHEMU97 catalogue of observations of the mutual phenomena of the Galilean satellites of Jupiter

Author

Arlot, J.-E., primary, Thuillot, W., additional, Ruatti, C., additional, Akasawa, H., additional, Baroni, S., additional, Beisker, W., additional, Berthier, J., additional, Blanco, C., additional, Boonstra, J., additional, Bourgeois, J., additional, Bulder, H., additional, Casas, R., additional, Castano, J. G., additional, Colas, F., additional, Collins, D., additional, Cuypers, J., additional, Czech, W., additional, D'Ambrosio, V., additional, Denzau, H., additional, Descamps, P., additional, Dimitrescu, A., additional, Dinakarian, N., additional, Dourneau, G., additional, Emelyanov, N., additional, Enriquez, J. M., additional, Fernandez, J. M., additional, Fernandez-Barba, D., additional, Flatres, T., additional, Foglia, S., additional, Goncalves, M., additional, Guhl, K., additional, Helmer, G., additional, Hirose, T., additional, Irsmambetova, T. R., additional, Krobusek, B. A., additional, Lecacheux, J., additional, Le Campion, J.-F., additional, Lou, M., additional, Mallama, A., additional, Marchis, F., additional, Navarro, M. A. S., additional, Nelson, P., additional, Okura, N., additional, Park, J., additional, Pauwels, T., additional, Pluchino, S., additional, Priban, V., additional, Rapaport, M., additional, Sacré, J.-J., additional, Salvaggio, F., additional, Sanchez, M. A., additional, Sanchez-Bajo, F., additional, Stefanescu, G., additional, Tanga, P., additional, Tejfel, V. G., additional, Trisan, J. L., additional, Trunkovsky, E. M., additional, Van Gestel, J., additional, Vandenbulcke, G., additional, Vasundhara, R., additional, Vass, G., additional, Vingerhoets, P., additional, Vu, D. T., additional, and Wilds, R. T., additional

Published
2006
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33. INTEGRAL observations of SS433: Results of a coordinated campaign

Author

Cherepashchuk, A. M., primary, Sunyaev, R. A., additional, Fabrika, S. N., additional, Postnov, K. A., additional, Molkov, S. V., additional, Barsukova, E. A., additional, Antokhina, E. A., additional, Irsmambetova, T. R., additional, Panchenko, I. E., additional, Seifina, E. V., additional, Shakura, N. I., additional, Timokhin, A. N., additional, Bikmaev, I. F., additional, Sakhibullin, N. A., additional, Aslan, Z., additional, Khamitov, I., additional, Pramsky, A. G., additional, Sholukhova, O., additional, Gnedin, Yu. N., additional, Arkharov, A. A., additional, and Larionov, V. M., additional

Published
2005
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34. The PHESAT95 catalogue of observations of the mutual events of the Saturnian satellites

Author

Thuillot, W., primary, Arlot, J.-E., additional, Ruatti, C., additional, Berthier, J., additional, Blanco, C., additional, Colas, F., additional, Czech, W., additional, Damani, M., additional, D'Ambrosio, V., additional, Descamps, P., additional, Dourneau, G., additional, Emelianov, N., additional, Foglia, S., additional, Helmer, G., additional, Irsmambetova, T. R., additional, James, N., additional, Laques, P., additional, Lecacheux, J., additional, Le Campion, J.-F., additional, Ledoux, C., additional, Le Floch, J.-C., additional, Oprescu, G., additional, Rapaport, M., additional, Riccioli, R., additional, Starosta, B., additional, Tejfel, V. G., additional, Trunkovsky, E. M., additional, Viateau, B., additional, Veiga, C. H., additional, and Vu, D. T., additional

Published
2001
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35. Mutual positions of the Galilean satellites of Jupiter from photometric observations during their mutual occultations and eclipses in 1997

Author

Emelianov, N. V., primary, Berejnoi, A. A., additional, Vashkovjak, S. N., additional, Glushkova, E. A., additional, Gorda, S. Yu., additional, Delets, A., additional, Dorokhova, T. N., additional, Dorokhov, N. I., additional, Esipov, V. F., additional, Izmailov, I. S., additional, Irsmambetova, T. R., additional, Kiselev, A. A., additional, Kiseleva, T. P., additional, Kornilov, V. G., additional, Kucherov, V., additional, Ledovskaya, I., additional, Mukhamednazarov, S., additional, Raskhozhev, V. N., additional, Tejfel, V. G., additional, and Charitonova, G. A., additional

Published
2000
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