dc.contributor.author |
Chaubey, U. S. |
|
dc.date.accessioned |
2010-08-17T09:14:48Z |
|
dc.date.available |
2010-08-17T09:14:48Z |
|
dc.date.issued |
1984 |
|
dc.identifier.citation |
This article is downloaded from ADS site |
en_US |
dc.identifier.uri |
http://hdl.handle.net/123456789/731 |
|
dc.description.abstract |
Twelve photoelectric light curves of six eclipsing binary stars namely GC Cas, WX Cep, UZ Cyg, VW Cyg, AQ Peg and ST Per in two different filters (B and V for the first five binaries and R and I for ST Per) have been analyzed by Kopal's new method of analysis of the light curves of eclipsing system in the frequency domain. The elements of the systems have been evaluated and their evolutionary status discussed. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
basi12-237 |
|
dc.subject |
Eclipsing binaries, Photometric elements, Absolute stellar dimensions, Stellar evolution |
en_US |
dc.title |
Revised elements and evolutionary status of six eclipsing binary stars |
en_US |
dc.type |
Article |
en_US |