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 |