首页 | 本学科首页   官方微博 | 高级检索  
     检索      

RT Leonis Minoris: an Unstable W Ursae Majoris System with a Spotted Component
作者姓名:Yu-Lan Yang and Qing-Yao LiuNational Astronomical Observatories  Yunnan Observatory  Chinese Academy of Sciences  Kunming  United Laboratory of Optical Astronomy  Chinese Academy of Sciences
作者单位:Yu-Lan Yang and Qing-Yao LiuNational Astronomical Observatories,Yunnan Observatory,Chinese Academy of Sciences,Kunming 650011; United Laboratory of Optical Astronomy,Chinese Academy of Sciences
基金项目:the National Natural Science Foundation of China.
摘    要:Complete BV light curves of the W UMa type binary RT LMi are presented. From the observations, four times of minimum light were determined. Based on the new times of minimum light and those collected from the literature, changes in the orbital period of the system were found and analyzed with Kalimeris et al.'s method. The result shows that the orbital period possibly oscillates with a cycle of about 64 years and an amplitude of 1.2 × 10-6 days. The present CCD photometric observations reveal that the light curves are obviously asymmetrical, and show a positive O'Connell effect, while the light curves obtained in 1982 exhibit a negative O'Connell effect. The present light curves were analyzed by means of the latest version of the Wilson-Devinney code, which was also used to correct the photometric effects, including the distortion on the radial-velocity curves obtained by Rucinski et al. The following absolute dimensions have been derived: MI -1.28 ±0.08 M⊙, M2 = 0.48 ±0.06 M⊙, R1 = 1.28 ±0.06 R⊙,

关 键 词:BV  光线曲率  放射性示踪物  狮子座  轨道周期

RT Leonis Minoris:an Unstable W Ursae Majoris System with a Spotted Component
Yu-Lan Yang and Qing-Yao LiuNational Astronomical Observatories,Yunnan Observatory,Chinese Academy of Sciences,Kunming , United Laboratory of Optical Astronomy,Chinese Academy of Sciences.RT Leonis Minoris:an Unstable W Ursae Majoris System with a Spotted Component[J].Chinese Journal of Astronomy and Astrophysics,2004,4(6):553-562.
Authors:Yu-Lan Yang and Qing-Yao LiuNational Astronomical Observatories  Yunnan Observatory  Chinese Academy of Sciences  Kunming  United Laboratory of Optical Astronomy  Chinese Academy of Sciences
Institution:Yu-Lan Yang and Qing-Yao LiuNational Astronomical Observatories,Yunnan Observatory,Chinese Academy of Sciences,Kunming 650011, United Laboratory of Optical Astronomy,Chinese Academy of Sciences
Abstract:
Keywords:star: contact binary - star: individuals: RT LMi - star: magnetic activity
本文献已被 CNKI 万方数据 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号