We discuss the evidence for GRS 1915 + 105 hosting an optically thick, relativistic accretion disk (at least in some spectral phases). We give particular emphasis to the iron line phenomenology. (C) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.
Martocchia, A., Belloni, T., Feroci, M., Karas, V., Matt, G. (2006). Understanding the relativistic accretion disk of GRS 1915+105. ADVANCES IN SPACE RESEARCH, 38(7), 1359-1364 [10.1016/j.asr.2005.03.146].
Understanding the relativistic accretion disk of GRS 1915+105
MATT, Giorgio
2006-01-01
Abstract
We discuss the evidence for GRS 1915 + 105 hosting an optically thick, relativistic accretion disk (at least in some spectral phases). We give particular emphasis to the iron line phenomenology. (C) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.File in questo prodotto:
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