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Galactic Wolf-Rayet stars in the mid-infrared
Published online by Cambridge University Press: 25 May 2016
Abstract
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We present the results of observations of a sample of Galactic WR stars with SCORE, the SIRTF Cornell Echelle spectrograph. Spectra with resolution R ≃ 600 and wavelength coverage from 7.5–15 μm were obtained for a variety of WR subtypes.
- Type
- Part 1. Basic observational properties of Wolf-Rayet stars and other hot massive stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
Van Cleve, J., Gull, G.E., Rinehart, S.A., Smith, J.D., Wilson, J.C, Houck, J.R., Brown, R., Blalock, W.
1998, PASP
110, 1479
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