We present new observations of the spectroscopic binary system HD 94546 and determine improved orbital parameters. HD 94546 is composed by a WN4 star and an O8V star with minimum masses mWR sen^3i ∼ 3 M⊙ and m0 sen^3i 6 M⊙.
Revista Mexicana de Astronomia y Astrofisica
- Pub Date:
- December 1985