BI VULPECULAE: A SIAMESE TWIN WITH TWO VERY SIMILAR COOL STARS IN SHALLOW CONTACT-Reference-Cited by-同舟云学术

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BI VULPECULAE: A SIAMESE TWIN WITH TWO VERY SIMILAR COOL STARS IN SHALLOW CONTACT

Published:2013-10-23 Issue:1 Volume:209 Page:13
ISSN:0067-0049
Container-title:The Astrophysical Journal Supplement Series
language:
Short-container-title:ApJS

Author:

Qian S.-B.,Liu N.-P.,Li K.,He J.-J.,Zhu L.-Y.,Zhao E. G.,Wang J.-J.,Li L.-J.,Jiang L.-Q.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/0067-0049/209/1/13/pdf

Reference76 articles.

1. A mechanism for orbital period modulation in close binaries

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

2. Periodic Variation Studies of the Two Short Period W UMa-type Eclipsing Binaries: LX Lyn and V0853 Aur;Research in Astronomy and Astrophysics;2024-01-01

3. A Study of Ten Early-type Contact Binary Stars in the Small Magellanic Cloud;Publications of the Astronomical Society of the Pacific;2023-09-01

4. NY Bootes: An Active Deep and Low-mass-ratio Contact Binary with a Cool Companion in a Hierarchical Triple System;The Astrophysical Journal;2023-08-28

5. OT UMa and 2MASS J09251388+6424488: Two active contact eclipsing binary systems;New Astronomy;2023-08

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