Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6402
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dc.contributor.authorRajamohan, R-
dc.date.accessioned2013-10-04T13:32:07Z-
dc.date.available2013-10-04T13:32:07Z-
dc.date.issued1973-
dc.identifier.citationAsundi, R.K., and Abhyankar, K.D eds. Proceedings of a Symposium on Spectroscopic Studies of Astrophysical Interest, 16 to 18 August 1972, pp. 109-120en
dc.identifier.urihttp://hdl.handle.net/2248/6402-
dc.descriptionOpen Accessen
dc.description.abstractFrom a measurement of the equivalent width of H alpha in the star gamma 1 Velorum, it is found that My (gamma1 Vel)=-3.1. Assummg gamma 1 and 2 Velorum are at the same distance, a distance modulus of 7.4 magnitudes for gamma., Velorum is obtained. From a study of the absorption lines of the 091 component and the emission lines in the infra-red of the We8 component the difference in magnitude between the two components is found to be about one magnitude. The 0 component is brighter and the derived magnitudes are Mv (WC8+09I)=- 5.6, MT (091)= -5.2 and Mv (WC8)=-4.2.en
dc.language.isoenen
dc.publisherCentre of Advanced Study in Astronomy, Osmania Universityen
dc.rights© Centre of Advanced Study in Astronomy,Osmania Universityen
dc.titleThe spectrum of gamma velorumen
dc.typeArticleen
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