Infrared excess in Wolf-Rayet stars

Details Infrared excess in Wolf-Rayet stars Infrared excess in Wolf-Rayet stars

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123..155s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 1, June 1986, p. 155-159.

Astronomy and Astrophysics

Astrophysics

1

Emission Spectra, Infrared Spectra, Spectral Energy Distribution, Stellar Temperature, Wolf-Rayet Stars, Continuous Spectra, Stellar Atmospheres, Stellar Models

Scientific paper

On the basis of continuum energy distributions in the wavelength region
λλ3200 - 11000 Å, effective temperatures 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.

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