The WN4+O8V spectroscopic binary HD 94546.

Niemela V. S.; Mandrini C. H.; Mendez R. H.

Vol. 11 No. 1 (1985), Research articles

Vol. 11 No. 1 (1985)

Research articles

The WN4+O8V spectroscopic binary HD 94546.

Published 1985-01-01

Niemela V. S.⁺⁻
Mandrini C. H.⁺⁻
Mendez R. H.⁺⁻

Niemela V. S.

-

Mandrini C. H.

-

Mendez R. H.

-

PDF

How to Cite

The WN4+O8V spectroscopic binary HD 94546. (1985). Revista Mexicana De Astronomía Y Astrofísica, 11(1), 143-147. https://astronomia.unam.mx/journals/rmxaa/article/view/1985rmxaa..11..143n

Abstract

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 m_WR sen^3i ∼ 3 M⊙ and m₀ sen^3i 6 M⊙.

The WN4+O8V spectroscopic binary HD 94546.

How to Cite

Download Citation

Abstract