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GRS 1915+105: Ten Years After

Tomaso Belloni
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Abstract

It is now ten years since the first microquasar GRS 1915+105 was discovered. More than six years of observations with RossiXTE have shown a level of variability never observed in any other X-ray source. Here I try to address some issues, based on X-ray observations only, that have relevance for theoretical modeling. First, I ignore these peculiarities and concentrate on the similarities with other X-ray transients. Then I focus on the peculiar variability and present a number of obervational facts that need to be addressed by theoretical models.

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Tomaso Belloni. 2002-08-06. GRS 1915+105: Ten Years After. https://arxiv.org/abs/astro-ph/0208129

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