Far infrared observations of Gamma Cassiopeiae from the IRAS satellite

Details Far infrared observations of Gamma Cassiopeiae from the IRAS satellite Far infrared observations of Gamma Cassiopeiae from the IRAS satellite

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98..334c&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, March 1986, p. 334-337.

Astronomy and Astrophysics

Astronomy

2

B Stars, Cassiopeia Constellation, Infrared Astronomy Satellite, Infrared Stars, Stellar Spectra, X Ray Binaries, Infrared Spectra, Spaceborne Astronomy, Stellar Atmospheres, Stellar Models, Stellar Temperature

Scientific paper

Detailed IRAS spectra are presented for the Be star Gamma Cas. The spectra are shown to be consistent with a Kurucz model atmosphere of 20,000 K and agree well with previous, less comprehensive observations. They confirm the existence of an infrared excess in this source, but do not agree in detail with the model of Poeckert and Marlborough (1978) based upon free-free emission from a circumstellar envelope.

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