Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/376
Title: Study of the Wolf-Rayet members of the cluster NGC 6231
Authors: Shylaja, B. S
Keywords: Emission Spectra;Open Clusters;Stellar Spectrophotometry;Wolf-Rayet Stars;Binary Stars;Light Curve;Spectral Energy Distribution;Stellar Atmospheres;Stellar Magnitude
Issue Date: Sep-1988
Publisher: Indian Academy Sciences
Citation: Journal of Astrophysics and Astronomy, Vol. 9, No. 3, pp. 161- 72
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.
URI: http://hdl.handle.net/2248/376
ISSN: 0250-6335
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Appears in Collections:IIAP Publications

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