Active M-type stars from the ultraviolet to the infrared

Details Active M-type stars from the ultraviolet to the infrared Active M-type stars from the ultraviolet to the infrared

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...244..433m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 244, no. 2, April 1991, p. 433-436. SERC-supported research.

Astronomy and Astrophysics

Astronomy

9

Black Body Radiation, Dwarf Stars, Emission Spectra, Infrared Astronomy, M Stars, Astronomical Photometry, H Alpha Line, Infrared Astronomy Satellite, Signal To Noise Ratios, Ultraviolet Radiation, Very Large Array (Vla)

Scientific paper

Fluxes at 12 microns are presented for a group of seven active dMe stars. Five of these stars are considered as significant detections at 25 microns, while only two stars were detected at 60 microns and only one at 100 microns. Comparing with previous results it is found that the fluxes are systematically lower by 7-50 percent depending on the band. Above 60 microns there is a definite excess over a blackbody radiation curve.

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