The 1999 Hercules X-1 anomalous low state

被引:33
作者
Coburn, W
Heindl, WA
Wilms, J
Gruber, DE
Staubert, R
Rothschild, RE
Postnov, KA
Shakura, N
Risse, P
Kreykenbohm, I
Pelling, MR
机构
[1] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
[2] Univ Tubingen, Inst Astron & Astrophys, D-72076 Tubingen, Germany
[3] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119899, Russia
[4] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
关键词
accretion; accretion disks; binaries : eclipsing; pulsars : individual (Hercules X-1); stars : neutron; X-rays : stars;
D O I
10.1086/317081
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A failed main-on in the 35 day cycle of Her X-l was observed with the Rossi X-Ray Timing Explorer on 1999 April 26. Exceptions to the normal 35 day cycle have been seen only twice before-in 1983 and again in 1993. We present timing and spectral results of this latest anomalous low state (ALS) along with comparisons to the main-on and normal low states. Pulsations were observed in the 3-18 keV band with a fractional rms variation of 0.037 +/- 0.003. Spectral analysis indicates that the ALS spectrum has the same shape as the main-on but is modified by heavy absorption and scattering. We find that 70% of the observed emission has passed through a cold absorber (N-H = 5.0 x 10(23) cm(-2)). This partially absorbing spectral fit can be applied to the normal low state with similar results. We find that the ALS observations may be interpreted as a decrease in inclination of the accretion disk causing the central X-ray source to be obscured over the entire 35 day cycle.
引用
收藏
页码:351 / 358
页数:8
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