dc.contributor.author |
Ashok, N. M. |
|
dc.contributor.author |
Bhatt, H. C. |
|
dc.contributor.author |
Kulkarni, P. V. |
|
dc.contributor.author |
Joshi, S. C. |
|
dc.date.accessioned |
2010-03-10T05:40:25Z |
|
dc.date.available |
2010-03-10T05:40:25Z |
|
dc.date.issued |
1984 |
|
dc.identifier.citation |
This article is downloaded for ADS |
en_US |
dc.identifier.uri |
http://hdl.handle.net/123456789/626 |
|
dc.description.abstract |
The Be stars as a class have been studied. JHK (1.2, 1.65, 2.2 μm) magnitudes for 55 Be stars are presented along with L (3.5 μm) magnitudes for 15 of them. For 20 Be stars the observations it is shown that the energy input to the circumstellar (CS) envelop. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
mn211-471 |
|
dc.subject |
Be stars - Infrared photometric |
en_US |
dc.title |
Infrared photometric studies of Be stars |
en_US |
dc.type |
Article |
en_US |