Infrared properties of CP stars

Details Infrared properties of CP stars Infrared properties of CP stars

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...67..195k&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 67, no. 2, Jan. 1987, p. 195-202.

Astronomy and Astrophysics

Astrophysics

17

Chemical Composition, Infrared Spectra, Peculiar Stars, Stellar Spectra, Radiant Flux Density, Spectrum Analysis, Stellar Envelopes, Stellar Magnitude

Scientific paper

Seventeen chemically peculiar stars of type CP2 and CP4 have been observed in the infrared bands J, H, K, L and M. Flux excesses in the M-band, previously reported by Groote and Kaufmann (1983) could not be confirmed. A detector nonlinearity may be responsible for contradicting observational results. No indications for dust shells or other circumstellar matter around CP stars could be found. The photometric variability in the IR - if present - is smaller than about 0.05 magnitudes for the observed stars.

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