In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 137 ( 1990), p. 15-18
Abstract:
Time resolved U-filter lightcurves of stellar flares on the dM4e star AD Leo have been measured to determine the flare frequency for individual observing seasons between 1972 and 1988. This report adds new data for 1984-1988. We use the number of flares with energy larger than 10∗∗30 erg, and the number of flare maxima with amplitudes larger than 0.3 as separate parameters to estimate flare frequencies. Chi-square tests do not reveal statistically significant variations of the flare frequency with time for 1972-1988.
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S0074180900187315
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1990
SSG:
16,12