IRAS excess radiation in Be stars and the behavior of the CA II triplet

Details IRAS excess radiation in Be stars and the behavior of the CA II triplet IRAS excess radiation in Be stars and the behavior of the CA II triplet

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...192..285j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988, p. 285, 286.

Astronomy and Astrophysics

Astronomy

5

B Stars, Calcium, Fine Structure, Infrared Astronomy Satellite, Near Infrared Radiation, Stellar Spectra, Line Spectra, Paschen Series

Scientific paper

The authors have examined a sample of 51 stars observed spectroscopically in the near infrared and by IRAS. They found an interesting correlation between the Ca II triplet emission and the IRAS excess: when the IRAS excess is large, Ca II is in emission; when the excess is small, no Ca II is present. This relation clarifies somewhat the erratic behavior of the Ca II triplet in the Be stars.

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