Cool Stellar Winds: Modeling of the Ultraviolet Resonance Lines to Derive Mass Loss Rates

Details Cool Stellar Winds: Modeling of the Ultraviolet Resonance Lines to Derive Mass Loss Rates Cool Stellar Winds: Modeling of the Ultraviolet Resonance Lines to Derive Mass Loss Rates

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baas...14..894d&link_type=gif

Bulletin of the American Astronomical Society, Vol. 14, p.894

Astronomy and Astrophysics

Astronomy

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