The W-subtype active contact binary PZ UMa with a possible more massive tertiary component-Reference-Cited by-同舟云学术

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The W-subtype active contact binary PZ UMa with a possible more massive tertiary component

Published:2019-02-11 Issue:2 Volume:71 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Zhou Xiao¹²³⁴,Soonthornthum Boonrucksar²

Affiliation:

1. Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650216 Kunming, China

2. National Astronomical Research Institute of Thailand, 260 Moo 4, Donkaew, Mae Rim, Chiang Mai, 50180, Thailand

3. Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P. O. Box 110, 650216 Kunming, China

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

Funder

Chinese Natural Science Foundation

Yunnan Natural Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/71/2/39/28537110/psz003.pdf

Reference53 articles.

1. The orbital elements of W Ursae Majoris systems

2. The ALADIN interactive sky atlas

3. On the properties of contact binary stars

Cited by 27 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The first study of the short period contact binary V415 Gem;New Astronomy;2024-10

2. A photometric study of a total-eclipse contact binary V458 Mon;New Astronomy;2024-10

3. Investigation of a W UMa-type contact binary GZ And in a physical triple system;Frontiers in Astronomy and Space Sciences;2024-07-15

4. V0405 Dra: A New Deep and Low Mass Ratio Contact Binary with Extremely Fast Decrease in the Orbital Period;Research in Astronomy and Astrophysics;2024-06-01

5. Investigation of an eclipsing binary star V1848 Orionis;New Astronomy;2024-05

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