Study of the Wolf-Rayet members of the cluster NGC 6231

dc.contributor.author	Shylaja, B. S
dc.date.accessioned	2005-03-03T06:55:27Z
dc.date.available	2005-03-03T06:55:27Z
dc.date.issued	1988-09
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 9, No. 3, pp. 161- 72	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/376
dc.description.abstract	Two Wolf-Rayet members of the cluster NGC 6231 are studied spectrophotometrically. HD 151932, a suspected variable, shows variations in the emission line flux as well as continuum magnitude measurements. An attempt is made to understand this variation as due to the asymmetric atmospheric structure. The other, HD 152270, a (WC7+O) binary, shows variation of emission line flux for C III and C IV lines only. This variation is studied as a possible phenomenon of atmospheric eclipses.	en
dc.format.extent	89046 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Academy Sciences	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1988JApA....9..161S
dc.subject	Emission Spectra	en
dc.subject	Open Clusters	en
dc.subject	Stellar Spectrophotometry	en
dc.subject	Wolf-Rayet Stars
dc.subject	Binary Stars
dc.subject	Light Curve
dc.subject	Spectral Energy Distribution
dc.subject	Stellar Atmospheres
dc.subject	Stellar Magnitude
dc.title	Study of the Wolf-Rayet members of the cluster NGC 6231	en
dc.type	Article	en