High amplitudeδScuti star BO Lyn with evidence of a late A-type companion in an elliptical orbit-Reference-Cited by-同舟云学术

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High amplitudeδScuti star BO Lyn with evidence of a late A-type companion in an elliptical orbit

Published:2018-01 Issue:1 Volume:18 Page:011
ISSN:1674-4527
Container-title:Research in Astronomy and Astrophysics
language:
Short-container-title:Res. Astron. Astrophys.

Author:

Li Lin-Jia,Qian Sheng-Bang,Zhang Jia,Zhu Li-Ying,Liao Wen-Ping

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1674-4527/18/i=1/a=011/pdf

Reference33 articles.

1. The first WASP public data release

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1. Observational constraints on a logarithmic scalar field dark energy model and black hole mass evolution in the Universe;The European Physical Journal C;2023-07-27

2. Revisiting bright δ Scuti stars and their period–luminosity relation with TESS and Gaia DR3;Monthly Notices of the Royal Astronomical Society;2022-07-31

3. CSS J213934.3-050020: A New Double-mode High-amplitude δ Scuti-type Pulsating Star;Publications of the Astronomical Society of the Pacific;2021-04-29

4. Photometric investigation of the eclipsing binary TX Herculis observed by LUT;Research in Astronomy and Astrophysics;2019-07-01

5. Identification and period investigation of pulsation variable star UY Camelopardalis, an RR Lyrae star in binary system;Publications of the Astronomical Society of Japan;2018-06-01

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