HL Aurigae: A pre-contact binary system with a solar-mass companion

HL Aurigae: A pre-contact binary system with a solar-mass companion

Orbital period changes of the near-contact binary (NCB) system, HL Aurigae, are analyzed based upon all the published CCD and photoelectric times of light minimum. It is found that the period of HL Aurigae shows a small-amplitude cyclic oscillation with a period of 6.5 years and an amplitude of 0.d0...

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書目詳細資料
Main Authors:	S. B. Qian, L. Y. Zhu, S. Boonruksar
格式:	雜誌
出版:	2018
主題:	Earth and Planetary Sciences Physics and Astronomy
在線閱讀:	https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=33645997353&origin=inward http://cmuir.cmu.ac.th/jspui/handle/6653943832/61635
標簽:	添加標簽沒有標簽, 成為第一個標記此記錄!
機構:	Chiang Mai University

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