Infrared excess in Wolf-Rayet stars

dc.contributor.author	Singh, M.
dc.date.accessioned	2010-02-16T10:56:15Z
dc.date.available	2010-02-16T10:56:15Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/528
dc.description.abstract	On the basis of continuum energy distributions in the wavelength region λ λ3200-11000 Å, effective temperature for 14 Wolf-Rayet stars are estimated by comparing with Kurucz (1979) model atmospheres. The continuum energy distribution curve shows strong infrared excess emissions above of λ5000 Å in every star.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	apss123-155
dc.subject	Wolf-Rayet stars	en_US
dc.title	Infrared excess in Wolf-Rayet stars	en_US
dc.type	Article	en_US