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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2524
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dc.contributor.authorKilambi, G. C-
dc.contributor.authorNagar, P-
dc.contributor.authorKameswara Rao, N-
dc.date.accessioned2008-06-27T09:42:28Z-
dc.date.available2008-06-27T09:42:28Z-
dc.date.issued1992-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 13, No. 2, pp. 175 - 194en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2524-
dc.description.abstractMid-ultraviolet and optical photometric analysis of helium stars are presented. A linear relation exists between the effective temperature derived from model atmospheres and (1965-V)0 index. The effective temperatures derived from (1965-V)0 index are somewhat higher than that of MK spectral type estimates especially for late B-type helium objectsen
dc.format.extent1339465 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992JApA...13..175Ken
dc.subjectASTRONOMICAL PHOTOMETRYen
dc.subjectB STARSen
dc.subjectSTELLAR ATMOSPHERESen
dc.subjectSTELLAR SPECTRAen
dc.subjectSTELLAR TEMPERATUREen
dc.subjectULTRAVIOLET ASTRONOMYen
dc.subjectHELIUMen
dc.subjectRADIANT FLUX DENSITYen
dc.subjectULTRAVIOLET SPECTRAen
dc.titleMid-ultraviolet and optical photometry of helium starsen
dc.typeArticleen
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