Infrared photometric studies of Be stars

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