Ta. Fleming et al., CORRELATIONS OF CORONAL X-RAY-EMISSION WITH ACTIVITY, MASS, AND AGE OF THE NEARBY K-DWARFS AND M-DWARFS, The Astrophysical journal, 450(1), 1995, pp. 401-410
Using the ROSAT telescope, we have detected X-ray emission from 87% of
all known K and M dwarfs within 7 pc of the Sun. Analysis of this vol
ume-limited sample of K and M dwarfs reveals no evidence for a decreas
e in coronal heating efficiency (as measured by L(X)/L(bol)) among the
lowest mass, presumably fully convective, late-M dwarfs. Furthermore,
our results indicate that those stars which exhibit little chromosphe
ric activity (i.e., dM and dK stars) do indeed have cooler and weaker
coronae than the more active dMe stars. While we also see a correlatio
n between coronal temperature/strength and metallicity (and presumably
age), no such correlation is seen with kinematic class. The latter re
sult leads us to suggest that kinematic class is a poor age indicator
for the nearby stars.