Quick search Find article
Quick search
Find article

Using the Galactic Dynamics of M7 Dwarfs to Infer the Evolution of Their Magnetic Activity

FREE ISSUE

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 affiliations


We 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.


Keywords

Galaxy: kinematics and dynamics; Galaxy: structure; solar neighborhood; stars: activity; stars: late-type; stars: low-mass, brown dwarfs


Dates

Issue 6 (2006 December)

Received 2006 June 30, accepted for publication 2006 August 25

Published 2006 November 1



View by subject




Export








Please login to access our web services, or create an account if you don't yet have one.

You must have cookies enabled in your web browser to be able to login.

Username
Password

Forgotten your password? Get a new one here.