dc.contributor.author |
Chaubey, U. S. |
|
dc.contributor.author |
Singh, M. |
|
dc.date.accessioned |
2010-07-19T07:10:32Z |
|
dc.date.available |
2010-07-19T07:10:32Z |
|
dc.date.issued |
1984 |
|
dc.identifier.citation |
This article is downloaded from ADS site |
en_US |
dc.identifier.uri |
http://hdl.handle.net/123456789/708 |
|
dc.description |
Restricted Access |
|
dc.description.abstract |
UBV light curves of the eclipsing binary systems V364 Cas and MM Cas are presented. A total of eight photoelectric times of minimum light for these stars were derived. The UBV photometric data of V364 Cas that the orbital period of the system given by Perova (1957) should be doubled. The secondary minimum falls at 0ᴾ.5. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
basi12-40 |
|
dc.subject |
Eclipsing binary, UBV light curve, Light elements |
en_US |
dc.title |
UBV photometry of two eclipsing binary stars |
en_US |
dc.type |
Article |
en_US |