Near infrared spectrometry of WC stars

Details Near infrared spectrometry of WC stars Near infrared spectrometry of WC stars

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192p..25w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Aug. 1980, p. 25P-30P.

Astronomy and Astrophysics

Astronomy

11

Emission Spectra, Hot Stars, Infrared Spectrometers, Line Spectra, Near Infrared Radiation, Stellar Spectrophotometry, Wolf-Rayet Stars, Helium, Infrared Filters

Scientific paper

Low resolution spectra of Wolf-Rayet stars in the 1.4 to 2.5 microns region are shown to be dominated by He I and He II blends at 1.87 micron and, in the WC stars only, by a He I line at 2.058 microns. The WC stars also show strong unidentified features at 1.72 and 2.41 microns. The (H-K) differences between WN and WC stars are attributed to the influence of the emission lines.

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