CP PUPPIS AND V1500 CYGNI

被引：22

作者：

WARNER, B

机构：

[1] Department of Astronomy, University of Cape Town, CP, Rondebosch,7700, South Africa

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1985年 / 217卷 / 01期

关键词：

Astrophysics; -; NASA;

D O I：

10.1093/mnras/217.1.1P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Photometric observations of CP Puppis (Nova Puppis 1942) show recurrent humps with a period of 0.06614 day (or its 1-day alias 0.06196 day). The orbital light curve is very similar to that of V1500 Cyg (Nova Cygni 1975); both stars were very fast novae of exceptionally large amplitude.The photometric period of CP Puppis is significantly different from the recently reported spectroscopic period which may indicate a 'superhump' or 'intermediate polar' model for the system. © 1985 Royal Astronomical Society. Provided by the NASA Astrophysics Data System.

引用

页码：P1 / P5

页数：5

共 30 条

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[2]

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[3]

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[4]

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