| 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 |