Advective Flow Paradigm And Microquasar GRS1915+105

2000/12/29 by Sandip K. Chakrabarti, Chakrabarti, Sandip K.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0012524

Kluwer Style Latex paper

arxiv created 2000/12/29 · arxiv updated 2009/12/01

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.

Related

• Advective Disks
• Non-linear variability in microquasars in relation with the winds from their accretion disks
• Advection-Dominated Accetion Flows
• Fundamental States of Accretion/Jet Configuration and the Black Hole Candidate GRS1915+105
• Understanding Galactic Black Hole Candidate GRS 1915+105