The Turbulent
Dynamo and X-ray Flux in Stars
¥We use simple stellar structure theory (MLT) to scale our simulations to
the outer layers of main sequence
stars (in the F0 to M0 spectral range) --- this allows us to estimate the unsigned flux
on the surface of Ònon-rotatingÓ reference stars.
¥With these estimates, we use the empirical relationship of Pevtsov et al.
(2003) to estimate the amount of
X-ray emission resulting from such a turbulent dynamo.