Ultraviolet flare activity on the eclipsing binary SZ PISCIUM

Details Ultraviolet flare activity on the eclipsing binary SZ PISCIUM Ultraviolet flare activity on the eclipsing binary SZ PISCIUM

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..522d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 283, no. 2, p. 522-524

Astronomy and Astrophysics

Astronomy

9

Chromosphere, Eclipsing Binary Stars, Stellar Coronas, Stellar Flares, Ultraviolet Astronomy, Ultraviolet Spectra, Astronomical Spectroscopy, Iue, Spectrum Analysis

Scientific paper

The estimated total chromospheric, transition region and coronal losses for a flare observed on the eclipsing binary SZ Psc with the International Ultraviolet Explorer (IUE) satellite on 6 July 1990 is of the order of 4.5 1036 ergs. This estimate is similar to that derived by Doyle et al. (1989) for an ultraviolet flare on another RS CVn star, II Peg, and is a substantial fraction of the total amount that is possible to store on these stars without having to evoke the presence of kiloGauss fields.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet flare activity on the eclipsing binary SZ PISCIUM does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Ultraviolet flare activity on the eclipsing binary SZ PISCIUM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet flare activity on the eclipsing binary SZ PISCIUM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1870058