IRAS observations of CP stars

Details IRAS observations of CP stars IRAS observations of CP stars

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...181..315k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 181, no. 2, July 1987, p. 315-322.

Astronomy and Astrophysics

Astronomy

14

Infrared Astronomy, Peculiar Stars, Spaceborne Astronomy, Stellar Composition, Astronomical Photometry, Cosmic Dust, Infrared Astronomy Satellite, Shell Stars, Stellar Envelopes

Scientific paper

IRAS data are presented which indicate that the IR part of the flux distribution of CP2 and CP3 stars is not affected by their chemical peculiarity. In CP4 stars, the two low temperature dust shells found are very similar to known shell stars, perhaps thereby indicating some physical relation between CP and Be stars. The present use of the IR flux as an indicator of CP star atmosphere thermal characteristics facilitates the study of physical changes in these atmospheres without interference from the individual abundance patterns of the stars.

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