The X-ray flare and the quiescent emission from Algol as detected by EXOSAT

Details The X-ray flare and the quiescent emission from Algol as detected by EXOSAT The X-ray flare and the quiescent emission from Algol as detected by EXOSAT

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...213..245v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 213, no. 1-2, April 1989, p. 245-260. Research supported by SRON.

Astronomy and Astrophysics

Astrophysics

99

Exosat Satellite, Stellar Coronas, Stellar Flares, Stellar Spectra, X Ray Sources, Coronal Loops, Eclipsing Binary Stars, Proportional Counters, Stellar Magnetic Fields, X Ray Spectroscopy

Scientific paper

The Algol system was observed on August 18/19,1983 with different combinations of three instruments aboard EXOSAT: the low-energy channel multiplier array, the medium-energy proportional counters, and the transmission grating spectrometer. The X-ray flare observed on August 19 was analyzed and the decay phase was studied. It is shown that during this phase the flare cools quasistatically according to the scaling laws and analytical expressions for the time-evolution of the relevant physical quantities are presented.

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