RW Doradus: A solar-type shallow contact binary with a new orbital period investigation-Reference-Cited by-同舟云学术

RW Doradus: A solar-type shallow contact binary with a new orbital period investigation

Published:2019-01-23 Issue:2 Volume:71 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Sarotsakulchai Thawicharat¹²³^ORCID,Qian Sheng-Bang¹²⁴⁵,Soonthornthum Boonrucksar³,Fernández Lajús Eduardo⁶⁷,Liu Nian-Ping¹⁴⁵,Zhou Xiao¹⁴⁵,Zhang Jia¹⁴⁵,Liao Wen-Ping¹⁴⁵,Reichart Daniel E⁸,Haislip Joshua B⁸,Kouprianov Vladimir V⁸,Poshyachinda Saran³

Affiliation:

1. Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, China

2. University of Chinese Academy of Sciences, 19A Yuquan Road, Shijingshan, 100049 Beijing, China

3. National Astronomical Research Institute of Thailand, Ministry of Science and Technology, Bangkok, Thailand

4. Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650216 Kunming, China

5. Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, China

6. Facultad de Ciencias Astronómicas y Geofísicas – UNLP, 1900 La Plata, Buenos Aires, Argentina

7. Instituto de Astrofísica de La Plata – CONICET/UNLP, 1900 La Plata, Buenos Aires, Argentina

8. Department of Physics and Astronomy, University of North Carolina, CB #3255, Chapel Hill, NC 27599, USA

Funder

National Natural Science Foundation of China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/71/2/34/28463777/psy149.pdf

Reference81 articles.

1. A mechanism for orbital period modulation in close binaries

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3. Kepler-503b: An Object at the Hydrogen Burning Mass Limit Orbiting a Subgiant Star

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