Advective Flow Paradigm And Microquasar GRS1915+105

dc.creatorChakrabarti, Sandip K.
dc.date2000-12-29
dc.date.accessioned2026-07-07T01:57:11Z
dc.date.available2026-07-07T01:57:11Z
dc.descriptionAdvective 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.
dc.descriptionKluwer Style Latex paper
dc.identifierhttps://arxiv.org/abs/astro-ph/0012524
dc.identifierhttp://arxiv.org/abs/astro-ph/0012524
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2288
dc.subjectAstrophysics
dc.titleAdvective Flow Paradigm And Microquasar GRS1915+105
dc.typetext

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