Spectroscopic orbits for K giants β Reticuli and ν Octantis: What is causing a low-amplitude radial velocity resonant perturbation in ν Oct?

Spectroscopic orbits for K giants β Reticuli and ν Octantis: What is causing a low-amplitude radial velocity resonant perturbation in ν Oct?

New astrometric-spectroscopic orbital solutions for the single-line K-giant binaries β Reticuli (P ≈ 5.2 yr, e = 0.3346 ± 0.0004) and ν Octantis (P ≈ 2.9 yr, e = 0.2358 ± 0.0003) have been derived based on high-precision spectroscopic radial velocities (RVs) and the Hipparcos astrometry. For the cas...

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書目詳細資料
Main Authors:	Ramm D.J., Pourbaix D., Hearnshaw J.B., Komonjinda S.
格式:	Article
語言:	English
出版:	2014
在線閱讀:	http://www.scopus.com/inward/record.url?eid=2-s2.0-63549085532&partnerID=40&md5=7478b79f102d13ef991f9370a3bd0259 http://cmuir.cmu.ac.th/handle/6653943832/5920
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
語言:	English

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