Some infrared photometric characteristics of Be stars

dc.contributor.author	Goraya, P. S.
dc.date.accessioned	2010-03-04T06:41:51Z
dc.date.available	2010-03-04T06:41:51Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/606
dc.description.abstract	A photometric study of a large sample of Be stars is reported. Infrared homogeneous observational data in the JHKL system are used to derive some photometric characteristics of Be stars, as a class. New infrared observations of 34 Be stars are included in the present paper. Infrared two-colours diagrams are used to investigate the presence of infrared emission in Be stars. The origin of infrared excess in relation to Balmer line emission in Be stars is discussed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass112-203
dc.subject	Be stars	en_US
dc.title	Some infrared photometric characteristics of Be stars	en_US
dc.type	Article	en_US