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2. Observational study of the extremely slow nova V1280 Scorpii

Author

Naito, H., Mizoguchi, S., Arai, A., Tajitsu, A., Narusawa, S., Yamanaka, M., Fujii, M., Iijima, T., Kinugasa, K., Kurita, M., Nagayama, T., Yamaoka, H., and Sadakane, K.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present multi-color light curves and optical spectra of V1280 Scorpii obtained from 2007 to 2012. It is shown that V1280 Sco is the extremely slow nova and the mass of white dwarf appears to be $\sim$ 0.6 M$\odot$ or lower. Blue-shifted multiple absorption lines of Na {\sc i} D, Ca {\sc ii} HK, and He {\sc i*} are detected on high-resolution spectra. We also discuss that an approach using metastable He absorption lines is useful to investigate structures of nova shells., Comment: 4 pages, 3 figures, to appear in Stella Novae: Future and Past Decades, P. A. Woudt & V. A. R. M. Ribeiro (eds), ASPCS

Published
2013

3. Five-Year Optical and Near Infrared Observations of the Extremely Slow Nova V1280 Scorpii

Author

Naito, H., Mizoguchi, S., Arai, A., Tajitsu, A., Narusawa, S., Yamanaka, M., Fujii, M., Iijima, T., Kinugasa, K., Kurita, M., Nagayama, T., Yamaoka, H., and Sadakane, K.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present optical ($B$, $V$, $R_{\rm c}$, $I_{\rm c}$ and $y$) and near infrared ($J$, $H$ and $K_{\rm s}$) photometric and spectroscopic observations of a classical nova V1280 Scorpii for five years from 2007 to 2011. Our photometric observations show a declining event in optical bands shortly after the maximum light which continues $\sim$ 250 days. The event is most probably caused by a dust formation. The event is accompanied by a short ($\sim$ 30 days) re-brightening episode ($\sim$ 2.5 mag in $V$), which suggests a re-ignition of the surface nuclear burning. After 2008, the $y$ band observations show a very long plateau at around $y$ = 10.5 for more than 1000 days until April 2011 ($\sim$ 1500 days after the maximum light). The nova had taken a very long time ($\sim$ 50 months) before entering the nebular phase (clear detection of both [\ion{O}{iii}] 4959 and 5007) and is still continuing to generate the wind caused by H-burning. The finding suggests that V1280 Sco is going through the historically slowest evolution. The interval from the maximum light (2007 February 16) to the beginning of the nebular phase is longer than any previously known slow novae: V723 Cas (18 months), RR Pic (10 months), or HR Del (8 months). It suggests that the mass of a white dwarf in the V1280 Sco system might be 0.6 $M_\mathrm{\sun}$ or smaller. The distance, based on our measurements of the expansion velocity combined with the directly measured size of the dust shell, is estimated to be 1.1 $\pm$ 0.5 kpc., Comment: 17 pages, 14 figures, accepted for publication in A&A

Published
2012
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5. Lorentz anomaly in the semi-light-cone gauge superstrings

Author

Kunitomo, H. and Mizoguchi, S.

Subjects
High Energy Physics - Theory
Abstract

We study the Lorentz invariance of D=4 and 6 superstrings in the double-spinor formalism, which are equivalent to the D=4 and 6 superstrings in the pure-spinor formalism in the sense of the BRST cohomology. We first re-examine how the conformal and Lorentz anomalies appear in the D=4 and 6 Green-Schwarz superstrings in the semi-light-cone gauge in the framework of BRST quantization. We construct a set of BRST invariant Lorentz generators and show that they do not form a closed algebra, even cohomologically. We then turn to the construction of Lorentz generators in the D=4 and 6 double-spinor superstrings, and show that the Lorentz invariance is again anomalous. We also discuss the relation between the anomaly-free Lorentz generators in the lower-dimensional pure-spinor formalisms and that obtained in this paper., Comment: 20 pages, version published in Progress of Theoretical Physics

Published
2007
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6. D=5 Simple Supergravity on AdS_{3} x S^{2} and N=4 Superconformal Field Theory

Author

Fujii, A., Kemmoku, R., and Mizoguchi, S.

Subjects
High Energy Physics - Theory
Abstract

We study the Kaluza-Klein spectrum of D=5 simple supergravity on $S^2$ with special interest in the relation to a two-dimensional N=4 superconformal field theory. The spectrum is obtained around the maximally supersymmetric Freund-Rubin-like background $AdS_3\times S^2$ by closely following the well-known techniques developed in D=11 supergravity. All the vector excitations turn out to be ``(anti-)self-dual'', having only one dynamical degree of freedom. The representation theory for the Lie superalgebra $SU(1,1|2)$ is developed by means of the oscillator method. We calculate the conformal weight of the boundary operator by estimating the asymptotic behavior of the wave function for each Kaluza-Klein mode. All the towers of particles are shown to fall into four infinite series of chiral primary representations of $SU(1,1|2)\times SL(2,{\bf R})$ (direct product), or $OSp(2,2|2;-1)\cong SU(1,1|2)\times SL(2,{\bf R})$ (semi-direct product)., Comment: 34 pages, 7 figures, revised version

Published
1998
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7. More on the Similarity between D=5 Simple Supergravity and M Theory

Author

Mizoguchi, S. and Ohta, N.

Subjects
High Energy Physics - Theory
Abstract

It has been known that D=5 simple supergravity resembles D=11 supergravity in many respects. We present their further resemblances in (1) the duality groups upon dimensional reduction, and (2) the worldsheet structure of the solitonic string of the D=5 supergravity. We show that the D=3, G_{2(+2)}/SO(4) (bosonic) nonlinear sigma model is obtained by using Freudenthal's construction in parallel to the derivation of the D=3, E_{8(+8)}/SO(16) sigma model from D=11 supergravity. The zero modes of the string solution with unbroken (4,0) supersymmetry consist of three (non-chiral) scalars, four Majorana-Weyl spinors of the same chirality and one chiral scalar, which suggests a duality to a certain six-dimensional chiral string theory. The worldsheet gravitational anomaly indicates a quantum correction to the Bianchi identity for the dualized two-form gauge field in the bulk just like the M5-brane case., Comment: 12 pages, references added

Published
1998
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11. 026 Differential Effects on Urethral Function, Epithelial Morphology, and Molecular Profile in Two Different Rat Models of Stress Urinary Incontinence by Simulated Birth Trauma or Estrogen Deficiency

Author

Kurobe, M., primary, Takaoka, E., additional, Suzuki, T., additional, Mizoguchi, S., additional, Saito, T., additional, Cao, N., additional, Alexandre, C.E., additional, Gotoh, D., additional, Igarashi, T., additional, Inamura, S., additional, Ando, T., additional, Inai, H., additional, Uchida, K., additional, Miyazaki, J., additional, and Yoshimura, N., additional

Published
2022
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12. Regeneration of Trachea and Esophagus by Scaffold-Free Structure, Using Bio-3D Printer

Author

Machino, R., primary, Matsumoto, K., additional, Taniguchi, D., additional, Uchida, F., additional, Hara, R., additional, Oyama, S., additional, Moriyama, M., additional, Tsuchiya, T., additional, Miyazaki, T., additional, Tomoshige, K., additional, Doi, R., additional, Mizoguchi, S., additional, Matsumoto, T., additional, Nakayama, K., additional, and Nagayasu, T., additional

Published
2022
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21. Complete genome sequence of Pseudomonas aeruginosa PAO1, an opportunistic pathogen

Author

Stover, C. K., Pham, X. Q., Erwin, A. L., Mizoguchi, S. D., Warrener, P., Hickey, M. J., Brinkman, F.S. L., Hufnagle, W. O., Kowalik, D. J., Lagrou, M., Garber, R. L., Goltry, L., Tolentino, E., Westbrock-Wadman, S., Yuan, Y., Brody, L. L., Coulter, S. N., Folger, K. R., Kas, A., Larbig, K., Lim, R., Smith, K., Spencer, D., Wong, G. K.-S., Wu, Z., Paulsen, I. T., Reizer, J., Saier, M. H., Hancock, R. E. W., Lory, S., and Olson, M. V.

Subjects
Environmental issues, Science and technology, Zoology and wildlife conservation
Abstract

Author(s): C. K. Stover [1]; X. Q. Pham [2]; A. L. Erwin [1]; S. D. Mizoguchi [1]; P. Warrener [1]; M. J. Hickey [1]; F.S. L. Brinkman [3]; W. O. [...]

Published
2000
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22. A study of the stream degassing process : using the silver-oxygen system

Author

Mizoguchi, S.

Subjects
669
Abstract

The fundamental aspects of the stream degassing process involving the nucleation and growth of bubbles and the fluid-dynamics of two-phase flow were studied. Pure silver containing various quantities of dissolved oxygen under atmospheric pressure was discharged through a nozzle into a vacuum tank at various pressures. Techniques were developed to measure the rate of discharge and the static pressure of the stream in the nozzle. The stream behaviour downstream of the nozzle exit was observed by a high-speed cine camera. For the flow of oxygen-saturated silver it was found that at tank pressures of less than 200 mm Hg, bubbles nucleated in the nozzle and the flow became choked. The appearance of the stream emerging from the nozzle was a homogeneous bubbly flow. The same stream was metastable single-phase flow at tank pressures of greater than 300 mm Hg. It was also found that the streams of air-saturated silver showed an intermittent bubble growth outside the nozzle exit only at tank pressures of 10 mm Hg and bellow. A theory was developed to correlate the static pressure in the nozzle, the volume ratio of gas to liquid, and the mass flow rate. By using the theory together with the measurements of flow rate and pressure, choking was confirmed and the volume ratio of gas to liquid was evaluated. Nucleation and growth of bubbles were discussed. Assessment of the data indicated that heterogeneous nucleation on cavities on the nozzle wall was the most likely mechanism and that the growth rate of bubbles was suppressed by inertial or viscous effects. Bubble growth outside the nozzle was complex at low tank pressures because of a pressure discontinuity at the nozzle exit due to choking. At tank pressures of 200 and 300 mm Hg bubble growth was found to obey the parabolic law for diffusion control.

Published
1972

29. Disruption of eyelid and cornea morphogenesis by epithelial β-catenin gain-of-function

Author

Mizoguchi, S., Suzuki, K., Zhang, J., Yamanaka, O., Chia-yang Liu, Okada, Y., Miyajima, M., Kokado, M., Kao, W. W. Y., Yamada, G., and Saika, S.

Subjects
Epithelial-Mesenchymal Transition, Eyelids, Cell Differentiation, Gestational Age, Mice, Transgenic, eye diseases, Epithelium, Mice, Mutant Strains, Cornea, Mice, Pregnancy, Mutation, Morphogenesis, Animals, Keratin-5, Female, sense organs, Promoter Regions, Genetic, beta Catenin, Research Article, Cell Proliferation, Signal Transduction
Abstract

Purpose To examine the developmental pathobiology of the eyelid and the cornea caused by epithelial β-catenin gain-of-function (gof) during mouse embryogenesis. Methods Compound mutant mice (Ctnnb1GOFOSE, gof of β-catenin in the epidermis and the ocular surface epithelium) were generated by time-mating keratin 5-promoter-Cre recombinase (Krt5-Cre) and Ctnnb1fE3/WT (floxed exon 3 of Ctnnb1) mice. Eyes obtained from wild-type (WT) and mutant embryos at various gestation stages until E18.5 were examined with histology and immunohistochemistry. The ultrastructure of the ocular tissues of the E18.5 embryos was also examined. Results Expression of the gof-β-catenin mutant protein in the epidermis severely impaired eyelid morphogenesis at E15.5, E17.5, and E18.5. The mutant stroma exhibited impaired keratocyte differentiation with accelerated cell proliferation and reduction in the accumulation of collagen type I. The mutant embryos also showed hyperproliferative nodules in the ocular surface epithelia with anomaly of cornea-type epithelial differentiation and the absence of the epithelial basement membrane. Conclusions Expression of the gof-β-catenin mutant protein in basal epithelial cells disrupts eyelid and cornea morphogenesis during mouse embryonic development due to the perturbation of cell proliferation and differentiation of the epithelium and the neural crest-derived mesenchyme.

Published
2015

35. Survey of period variations of superhumps in SU UMa-type dwarf novae. VI. The sixth year (2013-2014)

Author

Kato T., Dubovsky P., Kudzej I., Hambsch F., Miller I., Ohshima T., Nakata C., Kawabata M., Nishino H., Masumoto K., Mizoguchi S., Yamanaka M., Matsumoto K., Sakai D., Fukushima D., Matsuura M., Bouno G., Takenaka M., Nakagawa S., Noguchi R., Iino E., Pickard R., Maeda Y., Henden A., Kasai K., Kiyota S., Akazawa H., Imamura K., De Miguel E., Maehara H., Monard B., Pavlenko E., Antonyuk K., Pit N., Antonyuk O., Baklanov A., Ruiz J., Richmond M., Oksanen A., Harlingten C., Shugarov S., Chochol D., Masi G., Nocentini F., Schmeer P., Bolt G., Nelson P., Ulowetz J., Sabo R., Goff W., Stein W., Michel R., Dvorak S., Voloshina I., Metlov V., Katysheva N., Neustroev V., Sjoberg G., Littlefield C., Dębski B., Sowicka P., Klimaszewski M., Curyło M., Morelle E., Curtis I., Iwamatsu H., Butterworth N., Andreev M., Parakhin N., Sklyanov A., Shiokawa K., Novák R., Irsmambetova T., Itoh H., Ito Y., Hirosawa K., Denisenko D., Kochanek C., Shappee B., Stanek K., Prieto J., Itagaki K., and Stubbings R.

Subjects
Novae, cataclysmic variables, Accretion, accretion disks, dwarf novae [Stars]
Abstract

© The Author 2014. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved. Continuing the project undertaken by Kato et al. (2009), we collected times of superhump maxima for 56 SU UMa-type dwarf novae mainly observed during the 2013-2014 season and characterized these objects. We detected negative superhumps in VW Hyi and indicated that the low number of normal outbursts in some supercycles can be interpreted as a result of disk tilt. This finding, combined with the Kepler observation of V1504 Cyg and V344 Lyr, suggests that disk tilt is responsible for modulating the outburst pattern in SU UMa-type dwarf novae. We also studied the deeply eclipsing WZ Sge-type dwarf nova MASTER OT J005740.99+443101.5 and found evidence of a sharp eclipse during the phase of early superhumps. The profile can be reproduced by a combination of the eclipse of the axisymmetric disk and the uneclipsed light source of early superhumps. This finding shows the lack of evidence for a greatly enhanced hot spot during the early stage of WZ Sge-type outburst. We detected growing (stage A) superhumps in MN Dra and give a suggestion that some of SU UMa-type dwarf novae situated near the critical condition of tidal instability may show long-lasting stage A superhumps. The large negative period derivatives reported in such systems can be understood as a result of the combination of stage A and B superhumps. Two WZ Sge-type dwarf novae, AL Com and ASASSN-13ck, showed a long-lasting (plateau-type) rebrightening. In the early phase of their rebrightenings, both objects showed a precursor-like outburst, suggesting that the long-lasting rebrightening is triggered by a precursor outburst.

Published
2014

37. Prominent activity of the blazar OJ 287 in 2005: XMM-Newton and multiwavelength observations

Author

Ciprini, S, Raiteri, C. M., Rizzi, N, Agudo, I, Foschini, L, Fiorucci, M, Takalo, L. O., Villata, M, Ostorero, Luisa, Sillanpaeae, A, Valtonen, M, Tosti, G, ALLER H, WAGNER S. J., Aller, M. F., Arai, A, Arkharov, A. A., Bach, U, Bakis, V, Bagaglia, M, Boettcher, M, Buemi, C, Carosati, D, Chen, W. P., Efimov, Y, Emmanoulopoulos, D, Erdem, A, Fuhrmann, L, Frasca, A, Fullhart, M, Goyal, A, Heidt, J, Hovatta, T, Hroch, F, Ibrahimov, M. A., Jilkov'A, L, Joshi, M, Kamada, M, Katsuura, M, Kinoshita, D, Kostov, A, Kotaka, D, Kovalev, Y. Y., Krejcov'A, T, Krichbaum, T, Krishna, G, Kurosaki, M, Kurtanidze, O, Laehteenmaeki, A, Lanteri, L, Larionov, V, Lee, C. U., Leto, P, Li, J, Lindfors, E, Muenz, F, Marilli, E, Matsubara, Y, Mizoguchi, S, Mondal, S, Nakamura, K, Nieppola, E, Nilsson, K, Nishiyama, S, Nucciarelli, G, Ogino, A, Ohlert, J, Oksanen, A, Ovcharov, E, Pak, S, Pasanen, M, Pullen, C, Pursimo, T, Ros, J. A., Sadakane, K, Sadun, A. C., Sagar, R, Sohn, B. W., Sumitomo, N, Tanaka, K, Trigilio, C, Torniainen, I, Tornikoski, M, Umana, G, Ungerechts, H, Valtaoja, E, Volvach, A, Webb, J. R., Wu, J, Yim, H. S., and Zhang, Y.

Published
2007

40. WEBT and XMM-Newton observations of 3C 454.3 during the post-outburst phase - Detection of the little and big blue bumps

Author

Raiteri, C. M., Villata, M., Larionov, V. M., Pursimo, T., Ibrahimov, M. A., Nilsson, K., Aller, M. F., Kurtanidze, O. M., Foschini, L., Ohlert, J., Papadakis, I. E., Sumitomo, N., Volvach, A., Aller, H. D., Arkharov, A. A., Bach, U., Berdyugin, A., Boettcher, M., Buemi, C. S., Calcidese, P., Charlot, P., Sanchez, A. J. Delgado, Di Paola, A., Djupvik, A. A., Dolci, M., Efimova, N. V., Fan, J. H., Forne, E., Gomez, C. A., Gupta, A. C., Hagen-Thorn, V. A., Hooks, L., Hovatta, T., Ishii, Y., Kamada, M., Konstantinova, T., Kopatskaya, E., Kovalev, Yu. A., Kovalev, Y. Y., Lahteenmaki, A., Lanteri, L., Le Campion, J. -F, Lee, C. -U, Leto, P., Lin, H. -C, Lindfors, E., Mingaliev, M. G., Mizoguchi, S., Nicastro, F., Nikolashvili, M. G., Nishiyama, S., Östman, L., Ovcharov, E., Paakkonen, P., Pasanen, M., Pian, E., Rector, T., Ros, J. A., Sadakane, K., Selj, J. H., Semkov, E., Sharapov, D., Somero, A., Stanev, I., Strigachev, A., Takalo, L., Tanaka, K., Tavani, M., Torniainen, I., Tornikoski, M., Trigilio, C., Umana, G., Vercellone, S., Valcheva, A., Volvach, L., Yamanaka, M., Raiteri, C. M., Villata, M., Larionov, V. M., Pursimo, T., Ibrahimov, M. A., Nilsson, K., Aller, M. F., Kurtanidze, O. M., Foschini, L., Ohlert, J., Papadakis, I. E., Sumitomo, N., Volvach, A., Aller, H. D., Arkharov, A. A., Bach, U., Berdyugin, A., Boettcher, M., Buemi, C. S., Calcidese, P., Charlot, P., Sanchez, A. J. Delgado, Di Paola, A., Djupvik, A. A., Dolci, M., Efimova, N. V., Fan, J. H., Forne, E., Gomez, C. A., Gupta, A. C., Hagen-Thorn, V. A., Hooks, L., Hovatta, T., Ishii, Y., Kamada, M., Konstantinova, T., Kopatskaya, E., Kovalev, Yu. A., Kovalev, Y. Y., Lahteenmaki, A., Lanteri, L., Le Campion, J. -F, Lee, C. -U, Leto, P., Lin, H. -C, Lindfors, E., Mingaliev, M. G., Mizoguchi, S., Nicastro, F., Nikolashvili, M. G., Nishiyama, S., Östman, L., Ovcharov, E., Paakkonen, P., Pasanen, M., Pian, E., Rector, T., Ros, J. A., Sadakane, K., Selj, J. H., Semkov, E., Sharapov, D., Somero, A., Stanev, I., Strigachev, A., Takalo, L., Tanaka, K., Tavani, M., Torniainen, I., Tornikoski, M., Trigilio, C., Umana, G., Vercellone, S., Valcheva, A., Volvach, L., and Yamanaka, M.

Abstract

Context. The quasar-type blazar 3C 454.3 was observed to undergo an unprecedented optical outburst in spring 2005, affecting the source brightness from the near-IR to the X-ray frequencies. This was first followed by a millimetric and then by a radio outburst, which peaked in February 2006. Aims. In this paper we report on follow-up observations to study the multiwavelength emission in the post-outburst phase. Methods. Radio, near-infrared, and optical monitoring was performed by the Whole Earth Blazar Telescope (WEBT) collaboration in the 2006-2007 observing season. XMM-Newton observations on July 2-3 and December 18-19, 2006 added information on the X-ray and UV states of the source. Results. The source was in a faint state. The radio flux at the higher frequencies showed a fast decreasing trend, which represents the tail of the big radio outburst. It was followed by a quiescent state, common at all radio frequencies. In contrast, moderate activity characterized the near-IR and optical light curves, with a progressive increase of the variability amplitude with increasing wavelength. We ascribe this redder-when-brighter behaviour to the presence of a ""little blue bump"" due to line emission from the broad line region, which is clearly visible in the source spectral energy distribution (SED) during faint states. Moreover, the data from the XMM- Newton Optical Monitor reveal a rise of the SED in the ultraviolet, suggesting the existence of a "" big blue bump"" due to thermal emission from the accretion disc. The X-ray spectra are well fitted with a power- law model with photoelectric absorption, possibly larger than the Galactic one. However, the comparison with previous X-ray observations would imply that the amount of absorbing matter is variable. Alternatively, the intrinsic X-ray spectrum presents a curvature, which may depend on the X-ray brightness. In this case, two scenarios are possible. i) There is no extra absorption, and the X-ray spectrum hardens at low, authorCount :76

Published
2007
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45. The WEBT Campaign on the Blazar 3C 279 in 2006

Author

Bottcher, M., primary, Basu, S., additional, Joshi, M., additional, Villata, M., additional, Arai, A., additional, Aryan, N., additional, Asfandiyarov, I. M., additional, Bach, U., additional, Bachev, R., additional, Berduygin, A., additional, Blaek, M., additional, Buemi, C., additional, Castro‐Tirado, A. J., additional, De Ugarte Postigo, A., additional, Frasca, A., additional, Fuhrmann, L., additional, Hagen‐Thorn, V. A., additional, Henson, G., additional, Hovatta, T., additional, Hudec, R., additional, Ibrahimov, M., additional, Ishii, Y., additional, Ivanidze, R., additional, Jelinek, M., additional, Kamada, M., additional, Kapanadze, B., additional, Katsuura, M., additional, Kotaka, D., additional, Kovalev, Y. Y., additional, Kovalev, Yu. A., additional, Kubanek, P., additional, Kurosaki, M., additional, Kurtanidze, O., additional, Lahteenmaki, A., additional, Lanteri, L., additional, Larionov, V. M., additional, Larionova, L., additional, Lee, C.‐U., additional, Leto, P., additional, Lindfors, E., additional, Marilli, E., additional, Marshall, K., additional, Miller, H. R., additional, Mingaliev, M. G., additional, Mirabal, N., additional, Mizoguchi, S., additional, Nakamura, K., additional, Nieppola, E., additional, Nikolashvili, M., additional, Nilsson, K., additional, Nishiyama, S., additional, Ohlert, J., additional, Osterman, M. A., additional, Pak, S., additional, Pasanen, M., additional, Peters, C. S., additional, Pursimo, T., additional, Raiteri, C. M., additional, Robertson, J., additional, Robertson, T., additional, Ryle, W. T., additional, Sadakane, K., additional, Sadun, A., additional, Sigua, L., additional, Sohn, B.‐W., additional, Strigachev, A., additional, Sumitomo, N., additional, Takalo, L. O., additional, Tamesue, Y., additional, Tanaka, K., additional, Thorstensen, J. R., additional, Tosti, G., additional, Trigilio, C., additional, Umana, G., additional, Vennes, S., additional, Vitek, S., additional, Volvach, A., additional, Webb, J., additional, Yamanaka, M., additional, and Yim, H.‐S., additional

Published
2007
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47. WEBT and XMM-Newton observations of 3C 454.3 during the post-outburst phase

Author

Raiteri, C. M., primary, Villata, M., additional, Larionov, V. M., additional, Pursimo, T., additional, Ibrahimov, M. A., additional, Nilsson, K., additional, Aller, M. F., additional, Kurtanidze, O. M., additional, Foschini, L., additional, Ohlert, J., additional, Papadakis, I. E., additional, Sumitomo, N., additional, Volvach, A., additional, Aller, H. D., additional, Arkharov, A. A., additional, Bach, U., additional, Berdyugin, A., additional, Böttcher, M., additional, Buemi, C. S., additional, Calcidese, P., additional, Charlot, P., additional, Delgado Sánchez, A. J., additional, Di Paola, A., additional, Djupvik, A. A., additional, Dolci, M., additional, Efimova, N. V., additional, Fan, J. H., additional, Forné, E., additional, Gomez, C. A., additional, Gupta, A. C., additional, Hagen-Thorn, V. A., additional, Hooks, L., additional, Hovatta, T., additional, Ishii, Y., additional, Kamada, M., additional, Konstantinova, T., additional, Kopatskaya, E., additional, Kovalev, Yu. A., additional, Kovalev, Y. Y., additional, Lähteenmäki, A., additional, Lanteri, L., additional, Le Campion, J.-F., additional, Lee, C.-U., additional, Leto, P., additional, Lin, H.-C., additional, Lindfors, E., additional, Mingaliev, M. G., additional, Mizoguchi, S., additional, Nicastro, F., additional, Nikolashvili, M. G., additional, Nishiyama, S., additional, Östman, L., additional, Ovcharov, E., additional, Pääkkönen, P., additional, Pasanen, M., additional, Pian, E., additional, Rector, T., additional, Ros, J. A., additional, Sadakane, K., additional, Selj, J. H., additional, Semkov, E., additional, Sharapov, D., additional, Somero, A., additional, Stanev, I., additional, Strigachev, A., additional, Takalo, L., additional, Tanaka, K., additional, Tavani, M., additional, Torniainen, I., additional, Tornikoski, M., additional, Trigilio, C., additional, Umana, G., additional, Vercellone, S., additional, Valcheva, A., additional, Volvach, L., additional, and Yamanaka, M., additional

Published
2007
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49. The radio delay of the exceptional 3C 454.3 outburst

Author

Villata, M., primary, Raiteri, C. M., additional, Aller, M. F., additional, Bach, U., additional, Ibrahimov, M. A., additional, Kovalev, Y. Y., additional, Kurtanidze, O. M., additional, Larionov, V. M., additional, Lee, C.-U., additional, Leto, P., additional, Lähteenmäki, A., additional, Nilsson, K., additional, Pursimo, T., additional, Ros, J. A., additional, Sumitomo, N., additional, Volvach, A., additional, Aller, H. D., additional, Arai, A., additional, Buemi, C. S., additional, Coloma, J. M., additional, Doroshenko, V. T., additional, Efimov, Yu. S., additional, Fuhrmann, L., additional, Hagen-Thorn, V. A., additional, Kamada, M., additional, Katsuura, M., additional, Konstantinova, T., additional, Kopatskaya, E., additional, Kotaka, D., additional, Kovalev, Yu. A., additional, Kurosaki, M., additional, Lanteri, L., additional, Larionova, L., additional, Mingaliev, M. G., additional, Mizoguchi, S., additional, Nakamura, K., additional, Nikolashvili, M. G., additional, Nishiyama, S., additional, Sadakane, K., additional, Sergeev, S. G., additional, Sigua, L. A., additional, Sillanpää, A., additional, Smart, R. L., additional, Takalo, L. O., additional, Tanaka, K., additional, Tornikoski, M., additional, Trigilio, C., additional, and Umana, G., additional

Published
2007
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