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High Quality Echelle Observations of T Tauri Stars

Published online by Cambridge University Press:  19 July 2016

G. Basri
G. Basri*
Affiliation:
Astronomy Department, University of California, Berkeley, California USA

Abstract

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This is a very brief review of the high resolution line profile work that has been done on very young stars. The spectral anamolies peculiar to these stars are mentioned, with some discussion of what may give rise to them. The Hα line is discussed most extensively, as the most work has been done with it. While progress has been made in understanding the general nature of T Tauri spectra, there are very large gaps in our current understanding of the emission lines from these stars.

Type
II. Pre-Main-Sequence Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 99 - 104
Copyright
Copyright © Kluwer 1988 

References

Appenzeller, I., Jancovics, I., Jetter, R., 1986, Astron. Ap. Supp. 64, 65.Google Scholar
Bertout, C., 1984, Rep. Prog. Phys. 47, 111.CrossRefGoogle Scholar
Bertout, C., Basri, G., Bouvier, J., 1988, Ap. J. (submitted) Google Scholar
Edwards, S., Cabrit, S., Strom, S.E., Strom, K.M., 1987, Ap. J. (in press) Google Scholar
Finkenzeller, U. and Basri, G., 1987, Ap. J. 318, 823.CrossRefGoogle Scholar
Hartmann, L., 1982, Ap. J. Supp. 48, 109.CrossRefGoogle Scholar
Mundt, R., 1984, Ap. J. 280, 749.CrossRefGoogle Scholar
Mundt, R. and Giampapa, M.S., 1982, Ap. J. 256, 156.CrossRefGoogle Scholar
Rydgren, A.E., Strom, S.E., Strom, K.M., 1976, Ap. J. Supp. 30, 307.CrossRefGoogle Scholar
Ulrich, R. and Knapp, G., 1985, preprint.Google Scholar