Period changes in the eclipsing binary DX Vel
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F13%3A00457417" target="_blank" >RIV/68378271:_____/13:00457417 - isvavai.cz</a>
Result on the web
<a href="http://www.konkoly.hu/cgi-bin/IBVS?6066" target="_blank" >http://www.konkoly.hu/cgi-bin/IBVS?6066</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Period changes in the eclipsing binary DX Vel
Original language description
Comparison of the old and new photometric observations of the eclipsing binary DX Vel revealed the long term orbital period decrease, caused either by the mass transfer/mass loss effects or the presence of the third component in the system.
Czech name
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Czech description
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Classification
Type
J<sub>ost</sub> - Miscellaneous article in a specialist periodical
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2013
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
0374-0676
e-ISSN
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Volume of the periodical
2013
Issue of the periodical within the volume
6066
Country of publishing house
HU - HUNGARY
Number of pages
5
Pages from-to
6001
UT code for WoS article
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EID of the result in the Scopus database
2-s2.0-85049331160