A Large X-ray Flare on σ2 Coronae Borealis Observed with EXOSAT
DOI: 10.1007/3-540-18653-0_182
Bibcode: 1987LNP...291..494V
Mewe, R.; Brinkman, A. C.; van den Oord, G. H. J.
South Africa, Australia
Abstract
We report the observation of a compact flare on σ2 Coronae Borealis. The energy requirements for the flare are discussed and we find that current-driven turbulence can produce heating fast enough. During the initial phase of the flare classical transport theory is not applicable.
1987
•
Cool Stars, Stellar Systems and the Sun
Exosat
1