Mass loss from Wolf-Rayet stars

dc.contributor.author	Singh, M.
dc.date.accessioned	2010-02-08T08:38:30Z
dc.date.available	2010-02-08T08:38:30Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/491
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