Advective Flow Paradigm And Microquasar GRS1915+105
| dc.creator | Chakrabarti, Sandip K. | |
| dc.date | 2000-12-29 | |
| dc.date.accessioned | 2026-07-07T01:57:11Z | |
| dc.date.available | 2026-07-07T01:57:11Z | |
| dc.description | 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. | |
| dc.description | Kluwer Style Latex paper | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0012524 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0012524 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2288 | |
| dc.subject | Astrophysics | |
| dc.title | Advective Flow Paradigm And Microquasar GRS1915+105 | |
| dc.type | text |