HE 2350-3908: a dwarf nova with a 78(m) orbital period

被引：0
|
作者：
Augusteijn, T [1 ]
Wisotzki, L [1 ]
机构：
[1] HAMBURGER STERNWARTE, D-21029 HAMBURG, GERMANY
来源：
ASTRONOMY & ASTROPHYSICS | 1997年 / 324卷 / 03期
关键词：
stars: individual: HE2350-3908/RX J2353.0-3852; cataclysmic variables;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present time resolved CCD photometry and spectroscopy of the cataclysmic variable HE2350-3908 discovered in the Hamburg/ESO survey. We find that the orbital period of this source is 78.2 min. This is the shortest orbital period known to date for a cataclysmic variable with a normal hydrogen-rich secondary. The optical spectrum and the orbital light curve of HE2350-3908 is very similar to WZ Sge, and we argue that the source is a dwarf nova type cataclysmic variable with a very low mass-transfer rate, and a long recurrence time.
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页码：L57 / L60
页数：4
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