dc.contributor.author |
Srivastava, J. B. |
|
dc.contributor.author |
Kandpal, C. D. |
|
dc.date.accessioned |
2010-02-10T10:55:58Z |
|
dc.date.available |
2010-02-10T10:55:58Z |
|
dc.date.issued |
1986 |
|
dc.identifier.uri |
http://hdl.handle.net/123456789/499 |
|
dc.description.abstract |
Photoelectric observations of WX Eridani in B and V filters have been discussed. The maximum magnitudes of the system are B= 9. ͫ 70 and V= 9. ͫ 46. the B-V colours of the components are 0. ͫ 16 and 0. ͫ 80 for the primary and the secondary, respectively, while their spectral types are A5 + K0. The period has been found to be constant and its revised values is
0. ͩ 82327076. |
en_US |
dc.language.iso |
en |
en_US |
dc.relation.ispartofseries |
apss121-301 |
|
dc.subject |
WX Eridani, Eclipsing Binary |
en_US |
dc.title |
BV observations of the eclipsing binary WX Eridani |
en_US |
dc.type |
Article |
en_US |