Three modes of long wavelength flaring from GRS 1915+105: implications for jet formation
| dc.creator | Eikenberry, Stephen | |
| dc.date | 2000-11-12 | |
| dc.date.accessioned | 2026-07-07T01:56:30Z | |
| dc.date.available | 2026-07-07T01:56:30Z | |
| dc.description | GRS 1915+105 has exhibited at least three modes of long-wavelength (infrared to radio) flares. Class A flares are the bright ($\sim 1$ Jy) radio events whose apparent superluminal motion in many ways defines the microquasars. Class B flares have intermediate ($\sim 50-300$ mJy) flux densities in the IR and radio, and are associated with hard X-ray dipping behaviors. Class C flares are faint ($\sim 5-50$ mJy) IR/radio events associated with soft X-ray dips. We discuss each of these classes and their inter-relationships. | |
| dc.description | 4 pages, 2 figures, to be published in `Proceedings of the Third Microquasar Workshop: Granada Workshop on galactic relativistic jet sources', Eds A. J.Castro-Tirado, J. Greiner and J. M. Paredes, Astrophysics and Space Science, in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0011230 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0011230 | |
| dc.identifier | Astrophys.Space Sci. 276 (2001) 101-104 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2024 | |
| dc.subject | Astrophysics | |
| dc.title | Three modes of long wavelength flaring from GRS 1915+105: implications for jet formation | |
| dc.type | text |