dc.contributor.author |
Chaubey, U. S |
|
dc.date.accessioned |
2005-12-06T11:41:51Z |
|
dc.date.available |
2005-12-06T11:41:51Z |
|
dc.date.issued |
1984-09 |
|
dc.identifier.citation |
BASI, Vol. 12, No. 3, pp. 237-248 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/629 |
|
dc.description.abstract |
Twelve photoelectric light curves of six eclipsing binary stars namely GG Cas, WX Cep, UZ Cyg, AQ Peg and ST Per in two different filetrs (B and V for the first five binaries and R and I for ST Per) have been analysed 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 |
dc.format.extent |
851965 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Eclipsing binaries |
en |
dc.subject |
Photometric elements |
en |
dc.subject |
Absolute stellar dimensions |
en |
dc.subject |
Stellar evolution |
en |
dc.title |
Revised elements and Evolutionary status of six eclipsing binary stars |
en |
dc.type |
Article |
en |