X-ray variability in a complete sample of soft X-ray selected AGN

被引:89
作者
Grupe, D
Thomas, HC
Beuermann, K
机构
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
[3] Univ Sternwarte, D-37083 Gottingen, Germany
关键词
accretion; accretion disks; galaxies : active; galaxies : nuclei of; galaxies : Seyfert; quasars : general;
D O I
10.1051/0004-6361:20000429
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present ROSAT All-Sky Survey and ROSAT pointed observations (PSPC and HRI) of a complete sample of 113 bright soft X-ray AGN selected from the ROSAT Bright Source Catalog. We compare these observations in order to search for extreme cases of flux and spectral X-ray variability - X-ray transient AGN. Three definite transients and one transient candidate are found. The other sources show amplitude variations typically by factors of 2-3 on timescales of years. We found that the variability strength on timescales of days is a function of the steepness of the X-ray spectrum: steeper X-ray objects show stronger variability than flat X-ray spectrum sources. We also present new HRI measurements of our extreme X-ray transients IC 3599 and WPVS007. We discuss possible models to explain the X-ray transience and the variabilities observed in the non-transient sources.
引用
收藏
页码:470 / 486
页数:17
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