Activity in late-type stars. IX. The weakest chromosphere M dwarf yet discovered : GL 105B.
Bibcode: 1993A&A...278..520B
Byrne, P. B.
United Kingdom
Abstract
We present an estimate of chromospheric radiative losses from the dM(e) star, Gl 105B, based on a measurement of the MgII h&k emission line flux, which indicates that this star has the weakest chromospheric heating rate yet found in any M dwarf and that it lies well below the 'basal' heating rate of derived by Schrijver (1987).
1993
•
Astronomy and Astrophysics
IUE
6