| dc.contributor.author | Abhyankar, K. D | |
| dc.contributor.author | Panchatsaram, T | |
| dc.date.accessioned | 2005-02-09T06:11:31Z | |
| dc.date.available | 2005-02-09T06:11:31Z | |
| dc.date.issued | 1982-12 | |
| dc.identifier.citation | BASI, Vol. 10, No. 4, pp. 315-322 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/349 | |
| dc.description.abstract | An analysis of the minimum-time data of AK Her and ER Ori revelas possible sinudodal variations in their orbital periods. In the case of AK Her we suspect two additional components; one of mass 0.2 to 0.4 MSun with a period of 62 yr and the other of mass 0.2 to 0.6 MSun with a period of 207 yr. The probable third mass in ER Ori is less than 0.6 MSun for i>or equal to 60 degree with a long-term period of 34.78 yr. | en |
| dc.format.extent | 586715 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | |
| dc.publisher | Astronomical Society of India | en |
| dc.subject | AK Her | en |
| dc.subject | ER Ori | en |
| dc.subject | minimum-time data | en |
| dc.title | Light-time effect in AK Her and ER Ori | en |
| dc.type | Article | en |