| dc.contributor.author | Srivastava, R. K. | |
| dc.date.accessioned | 2010-03-03T06:08:10Z | |
| dc.date.available | 2010-03-03T06:08:10Z | |
| dc.date.issued | 1985 | |
| dc.identifier.citation | This article is downloaded for ADS | en_US |
| dc.identifier.uri | http://hdl.handle.net/123456789/597 | |
| dc.description.abstract | Investigations of the eclipsing binary system AR Lacertae have been reported earlier by author (cf. Srivastava, 1981; 1983s; 1983b; 1984; Goraya and Srivastava, 1984). AR Lac is a well known radio flaring sources. Some evidence of spot activity (cf. Srivastava, 1981; 1984; Goraya and Srivastava 1984). Recently Walter et al. (1983) derived coronal structure of the components of the system from X-ray and UV observations. | en_US |
| dc.language.iso | en_US | en_US |
| dc.relation.ispartofseries | ibvs2761 | |
| dc.subject | Eclipsing binary system AR Lacertae | en_US |
| dc.title | Flare like activity of AR Lacertae in 1982 | en_US |
| dc.type | Article | en_US |