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The Rotation and Variability of T Tauri Stars: Results of Two Decades of Monitoring at Van Vleck Observatory

Published online by Cambridge University Press:  12 April 2016

W. Herbst
W. Herbst*
Affiliation:
Astronomy Dept., Wesleyan University, Middletown, CT 06459, USA

Abstract

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A brief history of photometric monitoring of T Tauri stars with a 0.6 m telescope at Wesleyan University is given. This is followed by discussion of three recent results: 1) the mass dependence of stellar rotation rates in the Orion Nebula Cluster, 2) a check on stellar radii estimates of pre-main sequence stars, and 3) the nature of a very peculiar object in NGC 2264.

Type
V. Variability Study
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 177 - 186
Copyright
Copyright © Astronomical Society of the Pacific 2001

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