BD 11522 HV 11110 A POSSIBLE FLARE STAR OF TYPE K2

Loading...
Thumbnail Image

Date

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

Description

Citation

Endorsement

Review

Supplemented By

Referenced By