Comment on the IRAS infrared spectrum of Zeta Puppis (O4 If)

Details Comment on the IRAS infrared spectrum of Zeta Puppis (O4 If) Comment on the IRAS infrared spectrum of Zeta Puppis (O4 If)

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142l..25w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 2, Jan. 1985, p. L25-L28.

Astronomy and Astrophysics

Astronomy

4

Hot Stars, Infrared Astronomy Satellite, Infrared Spectra, Stellar Coronas, Stellar Winds, X Ray Astronomy, Early Stars, Stellar Mass Ejection, Supergiant Stars

Scientific paper

The infrared spectrum of ζ Pup that was obtained with the IRAS satellite has recently been compared by Lamers, Waters, and Wesseleus (1984) with flux distributions from models with coronal zones. Here the authors reconsider the thick corona and warm wind models used by Lamers et al. to interpret the IRAS data and find them unable to explain the X-ray observations. The thin coronal models of Waldron, however, are found to be capable of fitting the IRAS data. The question of the presence of base coronal regions must be considered still open.

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