Mass loss from Wolf-Rayet stars

Details Mass loss from Wolf-Rayet stars Mass loss from Wolf-Rayet stars

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.120..115s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 120, no. 1, March 1986, p. 115-119.

Astronomy and Astrophysics

Astronomy

1

Magellanic Clouds, Stellar Mass Ejection, Stellar Winds, Ultraviolet Astronomy, Wolf-Rayet Stars, Iue, Stellar Luminosity, Stellar Spectrophotometry, Stellar Temperature

Scientific paper

Mass loss rates for 9 LMC WR stars are determined using IUE, UV, and
visible spectrophotometric observations. A good correlation of mass loss
rate with effective temperature and luminosity is indicated by the data,
in agreement with the theoretical predictions.

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