TY Pup: A Low-mass-ratio and Deep Contact Binary as a Progenitor Candidate of Luminous Red Novae-Reference-Cited by-同舟云学术

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TY Pup: A Low-mass-ratio and Deep Contact Binary as a Progenitor Candidate of Luminous Red Novae

Published:2018-10-12 Issue:5 Volume:156 Page:199
ISSN:1538-3881
Container-title:The Astronomical Journal
language:
Short-container-title:AJ

Author:

Sarotsakulchai T.,Qian S.-B.,Soonthornthum B.,Zhou X.,Zhang J.,Reichart D. E.,Haislip J. B.,Kouprianov V. V.,Poshyachinda S.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3881/156/i=5/a=199/pdf

Reference74 articles.

1. Orbital Solutions and Absolute Elements of the W UMa Binary MW Pavonis

2. A mechanism for orbital period modulation in close binaries

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1. Investigation of the stability of the extreme low mass ratio contact binaries SX Crv and XX Sex, which are analysed photometrically;Advances in Space Research;2024-10

2. 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

3. V2769 Orionis: A new low-mass-ratio and deep-contact binary;New Astronomy;2023-08

4. Photometric and Spectroscopic Studies of the Long-Period Low-Mass-Ratio Deep-Contact Binary KN Per;Publications of the Astronomical Society of the Pacific;2022-11-01

5. Photometric Analysis of Three Potential Red Nova Progenitors;Research in Astronomy and Astrophysics;2022-09-28

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