THREE-SITE PHOTOMETRIC MONITORING OF THE δ SCT-TYPE PULSATING STAR V1162 ORIONIS : PERIOD CHANGE AND ITS IMPLICATIONS FOR PRE-MAIN SEQUENCE EVOLUTION-Reference-Cited by-同舟云学术

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THREE-SITE PHOTOMETRIC MONITORING OF THE δ SCT-TYPE PULSATING STAR V1162 ORIONIS : PERIOD CHANGE AND ITS IMPLICATIONS FOR PRE-MAIN SEQUENCE EVOLUTION

Published:2016-10-31 Issue:5 Volume:49 Page:199-208
ISSN:1225-4614
Container-title:Journal of The Korean Astronomical Society
language:en
Short-container-title:Journal of The Korean Astronomical Society

Author:

KIM SEUNG-LEE,CHA SANG-MOK,LIM BEOMDU,LEE JAE WOO,LEE CHUNG-UK,LEE YONGSEOK,KIM DONG-JIN,LEE DONG-JOO,KOO JAE-RIM,HONG KYEONGSOO,RYU YOON-HYUN,PARK BYEONG-GON

Publisher

The Korean Astronomical Society

Subject

Astronomy and Astrophysics,Space and Planetary Science

Cited by 2 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. Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2;The Astronomical Journal;2021-10-25

2. Preliminary results of variable star search using KMTNet data;EPJ Web of Conferences;2017

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