| Автор | Wei, Jian-Yan |
| Автор | Jiang, Xiao-Jun |
| Автор | Zhou, Da-Wei Xu,Ai-Ying |
| Автор | Hu, Jing-Yao |
| Дата выпуска | 2001-12-01 |
| dc.description | 1RXS J232953.9+062814 was identified as a cataclysmic variable by Wei et al. (1999). Four low-resolution spectra of 1RXS J232953.9+062814 were obtained with the 2.16-m telescope of the National Astronomical Observatories, of which two were at outburst, and two were at quiescence. The system is about 16.8 B and 16.5 V at quiescence, and 12.6 B and 12.6 V at outburst. The quiescent spectra were dominated by double-peaked Balmer emissions, which indicates a hydrogen-rich system with a high-inclination accretion disc. MgH and TiO absorption bands appeared in the quiescent spectrum which implies a companion with a spectral type of early M dwarf. If we take it as an M0 dwarf, then the system is located at a distance of 350 pc with a proper motion velocity 150 km s<sup>−1</sup>. The superhump period of 0.046311 days was confirmed by our V photometry. The short period and the hydrogen-rich nature reveal that this system is another SU Ursae Majoris-type dwarf nova below the period minimum after V485 Centauri. 1RXS J232953.9+062814 is one of the most important systems for studying the evolutionary scenario of cataclysmic variables since it is much brighter than V485 Cen. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Копирайт | © 2001 IOP Publishing Ltd |
| Название | 1RXS J232953.9+062814: a New SU UMa Dwarf Nova below the Period Minimum |
| Тип | paper |
| DOI | 10.1088/1009-9271/1/6/483 |
| Print ISSN | 1009-9271 |
| Журнал | Chinese Journal of Astronomy and Astrophysics |
| Том | 1 |
| Первая страница | 483 |
| Последняя страница | 486 |
| Аффилиация | Wei, Jian-Yan; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 |
| Аффилиация | Jiang, Xiao-Jun; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 |
| Аффилиация | Zhou, Da-Wei Xu,Ai-Ying; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 |
| Аффилиация | Hu, Jing-Yao; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 |
| Выпуск | 6 |
