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Mass loss from Wolf-Rayet stars

Show simple item record Singh, M. 2010-02-08T08:38:30Z 2010-02-08T08:38:30Z 1986
dc.description.abstract 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 predications. en_US
dc.language.iso en en_US
dc.relation.ispartofseries apss120-115
dc.subject Stars, Wolf-Rayet Stars en_US
dc.title Mass loss from Wolf-Rayet stars en_US
dc.type Article en_US

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