BVR photometric study of NSVS 2607629. A high mass-ratio W-type W UMa system
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- 作者：Birol Gü ; rol ; a ; Birol.Gurol@ankara.edu.tr" class="auth_mail" title="E-mail the corresponding author ; Raul Michelb ; rmm@astro.unam.mx" class="auth_mail" title="E-mail the corresponding author
- 关键词：Stars ; Binaries ; eclipsing ; Stars ; Fundamental parameters ; Technique ; Photometry ; Stars ; Individual (NSVS 2607629)
- 刊名：New Astronomy
- 出版年：2017
- 出版时间：February 2017
- 年：2017
- 卷：51
- 期：Complete
- 页码：128-134
- 全文大小：916 K
文摘
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We present the first analysis of photometric observations of NSVS2607629.
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New light elements was obtained and found that the system is located near the short-period limit.
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We present method of getting crucial information about spot parameters.
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Secondary minima did not occur at phase 0.5P like the systems V407 Peg, LU Vir and HH Boo.
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The geometrical and physical parameters of the system were derived.
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