Some infrared photometric characteristics of Be stars

Details Some infrared photometric characteristics of Be stars Some infrared photometric characteristics of Be stars

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.112..203g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 112, no. 1, May 1985, p. 203-208.

Astronomy and Astrophysics

Astronomy

B Stars, Infrared Astronomy, Infrared Photometry, Stellar Spectrophotometry, Variable Stars, Balmer Series, Emission Spectra, Main Sequence Stars, Stellar Color

Scientific paper

A photometric study of a large sample of Be stars is reported. Infrared homogeneous observational data in the JHKL system are used to derive some photometric characteristics of Be stars, as a class. New infrared observations of 34 Be stars are included in the present paper. Infrared two-colour diagrams are used to investigate the presence of infrared emission in Be stars. The origin of infrared excess in relation to Balmer line emission in Be stars is discussed.

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