A Spitzer IRS Survey of Wolf-Rayet Stars at 10--20 Microns

Details A Spitzer IRS Survey of Wolf-Rayet Stars at 10--20 Microns A Spitzer IRS Survey of Wolf-Rayet Stars at 10--20 Microns

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..177i&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on a mid-infrared survey of Wolf-Rayet stars using the Spitzer
IRS/SH instrument for types WN4-WN7 and WC4-WC7. Strong emission line
spectra are seen, including forbidden emission lines. Surprisingly, the
WN stars appear to show broad emission ``bumps'' that may be consistent
with silicate dust grains.

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