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@article{1228666,
author = {Liška, Jiří},
article_number = {6119},
keywords = {V2294 Cyg; light time effect; binary star; eclipsing binary; photometry; third body},
language = {eng},
issn = {1587-2440},
journal = {Information Bulletin on Variable Stars},
title = {Light time effect in the system V2294 Cyg},
url = {http://www.konkoly.hu/cgi-bin/IBVS?6119},
volume = {2014},
year = {2014}
}
TY - JOUR
ID - 1228666
AU - Liška, Jiří
PY - 2014
TI - Light time effect in the system V2294 Cyg
JF - Information Bulletin on Variable Stars
VL - 2014
IS - 6119
SP - 1-5
EP - 1-5
SN - 15872440
KW - V2294 Cyg
KW - light time effect
KW - binary star
KW - eclipsing binary
KW - photometry
KW - third body
UR - http://www.konkoly.hu/cgi-bin/IBVS?6119
L2 - http://www.konkoly.hu/cgi-bin/IBVS?6119
N2 - Light Time Effect with an eight year period is proposed for the overcontact binary system V2294 Cyg as an explanation for variations in its O-C diagram. Preliminary parameters of three-body system were determined. The published orbital period of about 3 years of a third body as well as the other parameters, based on Kepler photometry, for the possible triple system V2294 Cyg (Conroy et al. 2014), were found to be less reliable.
ER -
LIŠKA, Jiří. Light time effect in the system V2294 Cyg. \textit{Information Bulletin on Variable Stars}. 2014, roč.~2014, č.~6119, s.~1-5. ISSN~1587-2440.
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