Helium emission in the spectrum of Kappa Canis Majoris

Details Helium emission in the spectrum of Kappa Canis Majoris Helium emission in the spectrum of Kappa Canis Majoris

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hesk.book.....b&link_type=abstract

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Astronomy and Astrophysics

Astrophysics

Helium, Spectral Emission, Stellar Spectra, Absorption Spectra, Astronomical Models, Astrophysics, H Alpha Line

Scientific paper

Coude spectra of kappa CMa in the red region showed H alpha and He 1 lambda lambda 5876,6678 in emission. Each of the lines had two emission components, but the helium lines had no detectable absorption feature in between. While the H alpha emission peaks were separated by 160 km/sec, the helium lines were separated by 400 km/sec. A simple model is proposed to account for the behavior of these emission lines.

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