ARIES-Institutional Digital Repository

Infrared photometric studies of Be stars

Show simple item record

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


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search ARIES-IDR


Advanced Search

Browse

My Account

Context