1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/376
Full metadata record
DC FieldValueLanguage
dc.contributor.authorShylaja, B. S-
dc.date.accessioned2005-03-03T06:55:27Z-
dc.date.available2005-03-03T06:55:27Z-
dc.date.issued1988-09-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 9, No. 3, pp. 161- 72en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/376-
dc.description.abstractTwo 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.extent89046 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Academy Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1988JApA....9..161S-
dc.subjectEmission Spectraen
dc.subjectOpen Clustersen
dc.subjectStellar Spectrophotometryen
dc.subjectWolf-Rayet Stars-
dc.subjectBinary Stars-
dc.subjectLight Curve-
dc.subjectSpectral Energy Distribution-
dc.subjectStellar Atmospheres-
dc.subjectStellar Magnitude-
dc.titleStudy of the Wolf-Rayet members of the cluster NGC 6231en
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Study of the Wolf-Rayet members of the cluster.pdf1.01 MBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.