Light time effect in the system V2294 Cyg
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00079292" target="_blank" >RIV/00216224:14310/14:00079292 - isvavai.cz</a>
Result on the web
<a href="http://www.konkoly.hu/cgi-bin/IBVS?6119" target="_blank" >http://www.konkoly.hu/cgi-bin/IBVS?6119</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Light time effect in the system V2294 Cyg
Original language description
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 3years 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.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
S - Specificky vyzkum na vysokych skolach
Others
Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Information Bulletin on Variable Stars
ISSN
1587-2440
e-ISSN
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Volume of the periodical
2014
Issue of the periodical within the volume
6119
Country of publishing house
HU - HUNGARY
Number of pages
5
Pages from-to
1-5
UT code for WoS article
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EID of the result in the Scopus database
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