Andrew A. West et al. 2006 The Astronomical Journal 132 2507 doi:10.1086/508652
Andrew A. West1,2, John J. Bochanski2, Suzanne L. Hawley2, Kelle L. Cruz3, Kevin R. Covey2, Nicole M. Silvestri2, I. Neill Reid4 and James Liebert5
Show affiliationsWe present a spectroscopic study and dynamical analysis of ~2600 M7 dwarfs. We confirm our previous finding that the fraction of magnetically active stars decreases with vertical distance from the Galactic plane. We also show that the mean luminosity of the Hα emission has a small but statistically significant decrease with distance. Using space motions for ~1300 stars and a simple one-dimensional dynamical simulation, we demonstrate that the drop in the activity fraction of M7 dwarfs can be explained by thin disk dynamical heating and a rapid decrease of magnetic activity at a mean stellar age of ~6-7 Gyr.
Galaxy: kinematics and dynamics; Galaxy: structure; solar neighborhood; stars: activity; stars: late-type; stars: low-mass, brown dwarfs
Issue 6 (2006 December)
Received 2006 June 30, accepted for publication 2006 August 25
Published 2006 November 1
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