2002年2月
IR Com: Deeply eclipsing dwarf nova below the period gap - A twin of HT Cas?
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
- ,
- ,
- 巻
- 54
- 号
- 1
- 開始ページ
- 79
- 終了ページ
- 85
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1093/pasj/54.1.79
- 出版者・発行元
- OXFORD UNIV PRESS
We observed an X-ray selected, deeply eclipsing cataclysmic variable IR Com (= S 10932). We detected an outburst occurring on 1996 January 1. The light curve of the outburst closely resembled that of a normal outburst of an SU UMa-type dwarf nova, rather than that of an intermediate polar. Time-resolved photometry during the outburst showed that eclipses became systematically deeper and narrower as the outburst faded. Full-orbit light curves in quiescence showed little evidence of orbital humps or asymmetry of the eclipses. In addition to the presence of high-low transitions in quiescence, the overall behavior of the outbursts and the characteristics of the eclipse profiles suggest that IR Com can be best understood as a twin of HT Cas, a famous eclipsing SU UMa-type dwarf nova with a number of peculiarities.
- リンク情報
- ID情報
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- DOI : 10.1093/pasj/54.1.79
- ISSN : 0004-6264
- eISSN : 2053-051X
- CiNii Articles ID : 10010811627
- Web of Science ID : WOS:000174212000011