The overall flux distribution of magnetic chemically peculiar stars

Details The overall flux distribution of magnetic chemically peculiar stars The overall flux distribution of magnetic chemically peculiar stars

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...242..199l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 242, no. 1, Feb. 1991, p. 199-205.

Astronomy and Astrophysics

Astrophysics

5

A Stars, Magnetic Stars, Peculiar Stars, Radiative Transfer, Stellar Temperature, Balmer Series, Infrared Photometry, Reference Atmospheres, Stellar Atmospheres, Stellar Luminosity

Scientific paper

The combination of the ultraviolet, visible and infrared fluxes shows that magnetic chemically peculiar stars present a bluer but brighter Balmer jump and similar ultraviolet fluxes when compared to normal stars with the same near infrared fluxes. Near infrared photometry confirms this behavior of the Balmer jump. These results could be interpreted in terms of ultraviolet flux redistribution decreasing with wavelength and principally located in the Balmer jump region, according to the light variation amplitudes which generally present their maximum in the Balmer jump region and their minimum in the infrared.

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