THE LONG-PERIOD AM HERCULIS-LIKE CATACLYSMIC VARIABLE RXJ-051541+0104.6

被引:22
作者
WALTER, FM
WOLK, SJ
ADAMS, NR
机构
[1] Earth and Space Sciences Department, State University of New York, Stony Brook
关键词
ACCRETION; ACCRETION DISKS; NOVAE; CATACLYSMIC VARIABLES STARS; INDIVIDUAL; (RXJ; 051541+0104.6); X-RAYS; STARS;
D O I
10.1086/175319
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a new cataclysmic variable system, RXJ 051541 + 0104.6. The optical spectrum has a blue continuum with superposed H I and He I and II emission lines. The soft X-ray spectrum is well fit with a 50 eV blackbody. The X-ray and optical data are suggestive of an AM Herculis system. The X-ray light curve shows extreme variability on timescales of seconds and suggests an orbital period of order 8 hr, nearly twice that of the longest cataloged AM Her period. When bright, the X-ray light curve breaks up into a series of discrete bursts, which may be due to accretion of dense blobs of material of similar to 10(17) g mass.
引用
收藏
页码:834 / 840
页数:7
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