dc.contributor.author |
Mohin, S |
|
dc.contributor.author |
Raveendran, A. V |
|
dc.contributor.author |
Mekkaden, M. V |
|
dc.date.accessioned |
2005-03-02T06:19:54Z |
|
dc.date.available |
2005-03-02T06:19:54Z |
|
dc.date.issued |
1980 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 3, pp. 1-5 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/371 |
|
dc.description.abstract |
UBV photometry of Zeta Aurigae during the 1977 and 1979-80 eclipses is presented. From an analysis of the available photometry, it is concluded that the long term intrinsic variation in the brightness of the late-type super giant companion, as claimed by various investigators, is far from certain. |
en |
dc.format.extent |
141925 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Eclipsing binaries |
en |
dc.subject |
Zeta Aurigae |
en |
dc.subject |
UBV Photometry |
en |
dc.subject |
Variable Stars |
en |
dc.title |
Photometry of Zeta Aurigae during the 1977 and 1979-80 Eclipses |
en |
dc.type |
Article |
en |