NASA NTRS · 19870029254
Coronae on stars
Abstract
Three lines of evidence are noted to point to a flare heating source for stellar coronae: a strong correlation between time-averaged flare energy release and coronal X-ray luminosity, the high temperature flare-like component of the spectral signature of coronal X-ray emission, and the observed short time scale variability that indicates continuous flare activity. It is presently suggested that flares may represent only the extreme high energy tail of a continuous distribution of coronal energy release events.
Keep this discovery
Explore connections, maps & timelines
Haisch, B. M.. 1986-03-01. Coronae on stars. https://ntrs.nasa.gov/citations/19870029254
Cite the original work for its findings. Save a collection to share your selection of sources.