BD 11522 HV 11110 A POSSIBLE FLARE STAR OF TYPE K2
Loading...
Date
Authors
Journal Title
Journal ISSN
Volume Title
Publisher
Observatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
Abstract
Unusually strong emission lines for a late type dwarf were noted for the star BD+1° 1522. It was also found to have variations in its spectrum we are inclined to consider it as a flare star that underwent during one of our exposures a sudden increase in b
