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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
Author(s) -
SeungLee Kim,
Sang-Mok Cha,
Beomdu Lim,
Jae Woo Lee,
Chung-Uk Lee,
Yongseok Lee,
Dong-Jin Kim,
Dong-Joo Lee,
JaeRim Koo,
Kyeongsoo Hong,
Yoon-Hyun Ryu,
Byeong-Gon Park
Publication year - 2016
Publication title -
journal of the korean astronomical society/journal of the korean astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.568
H-Index - 22
eISSN - 2288-890X
pISSN - 1225-4614
DOI - 10.5303/jkas.2016.49.5.199
Subject(s) - physics , astrophysics , amplitude , variation (astronomy) , star (game theory) , gravitational microlensing , period (music) , light curve , telescope , stars , astronomy , optics , acoustics

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