Support for a white dwarf in the Be star binary γ Cassiopeiae

被引:8
作者
Apparao, KMV [1 ]
机构
[1] Opp Cardinal Sch, Bombay 400051, Maharashtra, India
关键词
stars : gamma Cas; white dwarf; stars : emission line; Be stars; stars : binaries; stars : neutron;
D O I
10.1051/0004-6361:20011625
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The recently discovered orbital period for gamma Cas and the modulation period in X-rays and optical are consistent with the orbital period-spin period relation for white dwarfs derived from a similar relation found for Be star - neutron star binaries. This lends support for the existence of a white dwarf in the gamma Cas binary.
引用
收藏
页码:554 / 555
页数:2
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