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Advective Flow Paradigm And Microquasar GRS1915+105

Sandip K. Chakrabarti

astro-pharXiv:astro-ph/0012524

Abstract

Advective accretion disks and winds are the most self-consistent solutions today. We describe this paradigm briefly and show how it attempts to explain some of the interesting observations of the galactic microquasar GRS1915+105.

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