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Optical Monitoring of T Tauri Stars

Published online by Cambridge University Press:  12 April 2016

William Herbst
William Herbst*
Affiliation:
Van Vleck Observatory, Wesleyan University

Extract

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At the Van Vleck Observatory of Wesleyan University, Middletown, Connecticut, we have initiated a program of monitoring T Tauri stars with the 24-inch reflector (Perkin Telescope). During the first observing season, we have obtained UBVRI and Hα (30Å and 150Å) data for five stars: T Tau, RY Tau, SU Aur, RW Aur, and CO Ori. The data will be presented elsewhere (Herbst, Holtzman and Phelps, 1982). Here we re-port some of our conclusions.

Type
Session III: Observed Activity in Related Objects
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 501 - 502
Copyright
Copyright © Reidel 1983

References

Herbig, G.H. 1962, Adv. Astron. Astrophys. 1, 47.CrossRefGoogle Scholar
Herbst, W., Holtzman, J.A., and Phelps, B.E. 1982, A.J., submitted.Google Scholar
Kuan, P. 1976, Astrophys. J. 210, 129.CrossRefGoogle Scholar
Mundt, R. and Giampapa, M.S. 1982, Astrophys, J. 256, 156.Google Scholar
Worden, S.P., Schneeberger, T.J., Kuhn, J.R., and Africano, J.L. 1981, Astrophys. J. 244, 520.Google Scholar