Coordinated multiband observations of stellar flares

Details Coordinated multiband observations of stellar flares Coordinated multiband observations of stellar flares

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985msngr..39....9r&link_type=abstract

ESO Messenger (ISSN 0722-6691), March 1985, p. 9-12.

Astronomy and Astrophysics

Astronomy

5

Flare Stars, Stellar Activity, Stellar Flares, Stellar Spectra, Continuous Spectra, H Alpha Line, Infrared Spectra, Iue, Radio Astronomy, Ultraviolet Spectra

Scientific paper

The March 28, 1984 flare of AD Leo is characterized on the basis of observations obtained over the spectral range from 200 nm to 20 cm using the IUE, the VLA, and four ESO telescopes as part of a coordinated multiband international campaign. The data are presented graphically and discussed, with consideration of faint negative K-band events observed simultaneously with the optical flare; an H-alpha precursor with longer energy-release relaxation than in the U continuum; and remarkably enhanced UV continuum, Mg II doublet, and 260-nm Fe II blend during the last secondary optical peak.

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