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 |