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 |