X-Ray Spectral Behavior of the Relativistic Jet Source Cygnus X-3
| dc.creator | McCollough, M. L. | |
| dc.creator | Robinson, C. R. | |
| dc.creator | Zhang, S. N. | |
| dc.creator | Harmon, B. A. | |
| dc.creator | Paciesas, W. S. | |
| dc.creator | Dieters, S. | |
| dc.creator | Phengchamnan, S. | |
| dc.creator | Hjellming, R. M. | |
| dc.creator | Rupen, M. | |
| dc.creator | Mioduszewski, A. J. | |
| dc.creator | Waltman, E. B. | |
| dc.creator | Ghigo, F. D. | |
| dc.creator | Pooley, G. G. | |
| dc.creator | Fender, R. P. | |
| dc.creator | Cui, W. | |
| dc.creator | Trushkin, S. | |
| dc.date | 1998-11-03 | |
| dc.date.accessioned | 2026-07-07T02:28:53Z | |
| dc.date.available | 2026-07-07T02:28:53Z | |
| dc.description | Cyg X-3 is an unusual X-ray binary which shows remarkable correlative behavior between the hard X-ray, soft X-ray, and the radio. We present an analysis of these long term light curves in the context of spectral changes of the system. This analysis will also incorporate a set of pointed RXTE observations made during a period when Cyg X-3 made a transition from a quiescent radio state to a flaring state (including a major flare) and then returned to a quiescent radio state. | |
| dc.description | 4 pages, 4 color figures, epsfig.sty included. To appear in the 3rd INTEGRAL Workshop Proceedings (The Extreme Universe) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9811046 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9811046 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13253 | |
| dc.subject | Astrophysics | |
| dc.title | X-Ray Spectral Behavior of the Relativistic Jet Source Cygnus X-3 | |
| dc.type | text |