Infrared excess in Wolf-Rayet stars

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1986 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 123, pages 155-159 (issn: 0004-640X, eissn: 1572-946X,

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Authors: Mahendra Singh;

doi: 10.1007/bf00649131

Infrared excess in Wolf-Rayet stars

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Abstract

On the basis of continuum energy distributions in the wavelength region λλ3200–11 000 A, 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 A in every star.

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