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29 results on '"Martino D"'

6. STREGA@VST: Structure and Evolution of the Galaxy

Author

Marconi, M., primary, Musella, I., additional, Di Criscienzo, M., additional, Cignoni, M., additional, Dall’Ora, M., additional, Ripepi, V., additional, Bono, G., additional, Brocato, E., additional, Coppola, G., additional, Grado, A., additional, Limatola, L., additional, Moretti, M. I., additional, Raimondo, G., additional, Stetson, P. B., additional, Calamida, A., additional, Cantiello, M., additional, Capaccioli, M., additional, Cappellaro, E., additional, Cioni, M.-R. L., additional, Degl’Innocenti, S., additional, De Martino, D., additional, Di Cecco, A., additional, Ferraro, I., additional, Iannicola, G., additional, Prada Moroni, P. G., additional, Silvotti, R., additional, Buonanno, R., additional, Getman, F., additional, Napolitano, N. R., additional, Pulone, L., additional, and Schipani, P., additional

Published
2016
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10. Stellar and galactic environment survey (SAGE)

Author

Barstow, M. A., primary, Burleigh, M. R., additional, Bannister, N. J., additional, Lapington, J. S., additional, Kowalski, M. P., additional, Cruddace, R. G., additional, Wood, K. S., additional, Auchere, F., additional, Bode, M. F., additional, Bromage, G. E., additional, Gibson, B., additional, Cameron, A. C., additional, Cassatella, A., additional, Delmotte, F., additional, Ravet, M.-F., additional, Doyle, J. G., additional, Jeffery, C. S., additional, Gaensicke, B., additional, Jordan, C., additional, Kappelmann, N., additional, Werner, K., additional, Lallement, R., additional, de Martino, D., additional, Matthews, S. A., additional, Phillips, K. J. H., additional, Del Zanna, G., additional, Orio, M., additional, Pace, E., additional, Pagano, I., additional, Schmitt, J. H. M. M., additional, and Welsh, B. Y., additional

Published
2008
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14. NON-COSMIC ABUNDANCES IN THE POLAR BY CAM?

Author

MOUCHET, M., primary, BONNET-BIDAUD, J.-M., additional, BEUERMANN, K., additional, DE MARTINO, D., additional, FERLET, R., additional, FRIED, R., additional, GÄNSICKE, B., additional, HOWELL, S., additional, LECAVELIER DES ETANGS, A., additional, MUKAI, K., additional, PORQUET, D., additional, ROUEFF, E., additional, and SZKODY, P., additional

Published
2001
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24. Age-dependent Prognostic Significance of N-myc Copy Number in Neuroblastoma1

Author

Tonini, G. P., primary, Badiali, M., additional, Cavazzana, A., additional, Di Martino, D., additional, Dominici, C., additional, Fontana, V., additional, Iolascon, A., additional, Lanino, E., additional, Basso, G., additional, Pession, A., additional, Raschellá, G., additional, Strigini, P., additional, Sansone, R., additional, and De Bernardi, B., additional

Published
1990
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28. Small angle neutron scattering studies of critical phenomena in a three-component microemulsion.

Author

Kremer, F., Lagaly, G., Kawasaki, K., Lindman, B., Okabayashi, H., Seto, H., Komura, S., Wignall, G. D., Triolo, R., and Chillura-Martino, D.

Abstract

Critical density fluctuations of a "water-in-oil" microemulsion consisting of water, benzene, and BHDC (benzyldimethyl-n-hexadecyl ammonium chloride) have been observed near the phase boundary by a small-angle neutron scattering (SANS). The observed profiles were well described by the product of a form factor of spherical droplets and a structure factor, consisting of a term describing the inter-droplet correlations and also an Ornstein-Zernike component describing the droplet density fluctuations. Allowance was also made for the droplet polydispersity, though the width of the distribution turned out to be very small (1-2%). The observed temperature dependence of the osmotic compressibility was fitted using the crossover function proposed by Belyakov et al., and the Ginzburg numbers were obtained of the order 10−2. These results indicate that longrange inter-droplet forces are not significant in this system, which displays upper critical solution temperature (UCST) behavior. In contrast, previous studies of systems displaying with lower critical solution temperature (LCST) behavior [e.g. water, n-decane and AOT (dioctyl sulfosuccinate sodium salt)] indicate that long-range interactions appear to dominate the phase separation behavior. [ABSTRACT FROM AUTHOR]

Published
1997
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29. Phase resolved UV spectroscopy of RX J0019.8+2156.

Author

Araki, H., Brézin, E., Ehlers, J., Frisch, U., Hepp, K., Jaffe, R. L., Kippenhahn, R., Weidenmüller, H. A., Wess, J., Zittartz, J., Beiglböck, W., Greiner, Jochen, Gänsicke, B. T., Beuermann, K., and Martino, D.

Abstract

We present orbital phase-resolved UV spectroscopy of the supersoft X-ray source RX J0019.8+2156 obtained with IUE in 1992-93. The UV and optical light curves show a quasi-sinusoidal orbital modulation with wavelength dependent amplitude and a deep secondary minimum at Φ∼0.6. The UV spectrum is of lower excitation than in other SSS. The various metal absorption lines are consistent with the source being located outside the gas layer of the galactic disc, though there is some evidence for intrinsic absorption. The UV spectrum of RX J0019 differs from those of the LMC sources CAL 83 and RX J0513.9-6951. A simple model where the UV light originates from the hot primary, the accretion disk and the heated secondary fails to reproduce the observed UV continuum. [ABSTRACT FROM AUTHOR]

Published
1996
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