Unusual phase reversal of superhumps in ER Ursae Majoris

被引:13
|
作者
Kato, T [1 ]
Nogami, D
Masuda, S
机构
[1] Kyoto Univ, Dept Astron, Sakyo Ku, Kyoto 6068502, Japan
[2] Kyoto Univ, Hida Observ, Gifu 5061314, Japan
[3] Natl Astron Observ, Okayama Astrophys Observ, Okayama 7190232, Japan
关键词
accretion; accretion disks; stars : dwarf novae; stars : individual (ER Ursae Majoris); stars; novae; cataclysmic variables; stars : oscillations;
D O I
10.1093/pasj/55.2.L7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We studied the evolution of superhumps in the peculiar SU UMa-type dwarf nova, ER UMa. Contrary to the canonical picture of the SU UMa-type superhump phenomena, the superhumps of ER UMa show an unexpected phase reversal during the very early stage (similar to 5 d after the superoutburst maximum). We interpret that a sudden switch to so-called late superhumps occurs during the very early stage of a superoutburst. What had been believed to be (ordinary) superhumps during the superoutburst plateau of ER UMa were actually late superhumps. The implication of this discovery is briefly discussed.
引用
收藏
页码:L7 / L10
页数:4
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