Infrared colors of the chemically peculiar stars of the upper main sequence

Details Infrared colors of the chemically peculiar stars of the upper main sequence Infrared colors of the chemically peculiar stars of the upper main sequence

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...125...29b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 125, no. 1, Aug. 1983, p. 29-33.

Astronomy and Astrophysics

Astrophysics

17

A Stars, Infrared Stars, Main Sequence Stars, Peculiar Stars, Stellar Color, Stellar Spectrophotometry, Atmospheric Models, Stellar Atmospheres

Scientific paper

A program of J, H, K, L-prime, M photometry of CP stars and normal comparison stars has been carried out at the Mauna Kea Observatory. The infrared colors of the CP and normal stars are found to be similar to each other, and to the predictions of normal model atmospheres, to within at worst 20 percent. These results do not support the conclusion of Groote et al. (1980, 1981) that infrared excesses at 5 microns are found in CP stars with magnetic fields.

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