Evolution of spectral parameters during a pre-eclipse dip of Her X-1
| dc.creator | Stelzer, B. | |
| dc.creator | Wilms, J. | |
| dc.creator | Staubert, R. | |
| dc.creator | Gruber, D. | |
| dc.creator | Rothschild, R. | |
| dc.date | 1998-12-07 | |
| dc.date.accessioned | 2026-07-07T02:29:32Z | |
| dc.date.available | 2026-07-07T02:29:32Z | |
| dc.description | We report on a pre-eclipse dip of the X-ray binary Her X-1 observed by the Rossi X-ray Timing Explorer (RXTE) in July 1996. We present the evolution of the spectral parameters in the 3-18 keV range with a temporal resolution of 16 s and show that the varying flux of the spectrum can be interpreted solely by a time varying column density. We also find that the lightcurve is characterized by symmetric substructures with recurrence time of a few minutes that can be successfully modeled by Gaussian profiles. | |
| dc.description | 9 pages, 8 figures, accepted for publication in Astronomy & Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9812128 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9812128 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13509 | |
| dc.subject | Astrophysics | |
| dc.title | Evolution of spectral parameters during a pre-eclipse dip of Her X-1 | |
| dc.type | text |