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Galactic Wolf-Rayet stars in the mid-infrared

Published online by Cambridge University Press:  25 May 2016

John D. Smith
Affiliation:
Cornell University Department of Astronomy, Ithaca, NY 14853
Jim R. Houck
Affiliation:
Cornell University Department of Astronomy, Ithaca, NY 14853

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
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

van der Hucht, K.A., Morris, P.W., Williams, P.M., et al. 1996, A&A 315, L193 Google Scholar
Smith, J.D. et al. 1998, Proc. SPIE, 3354, 798 CrossRefGoogle Scholar
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 CrossRefGoogle Scholar