| dc.contributor.author | Rajamohan, R | |
| dc.date.accessioned | 2013-10-04T13:32:07Z | |
| dc.date.available | 2013-10-04T13:32:07Z | |
| dc.date.issued | 1973 | |
| dc.identifier.citation | Asundi, R.K., and Abhyankar, K.D eds. Proceedings of a Symposium on Spectroscopic Studies of Astrophysical Interest, 16 to 18 August 1972, pp. 109-120 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/6402 | |
| dc.description | Open Access | en |
| dc.description.abstract | From 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.iso | en | en |
| dc.publisher | Centre of Advanced Study in Astronomy, Osmania University | en |
| dc.rights | © Centre of Advanced Study in Astronomy,Osmania University | en |
| dc.title | The spectrum of gamma velorum | en |
| dc.type | Article | en |