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Spectroscopic Observations of Emission-line Stars

Published online by Cambridge University Press:  25 April 2016

T. Kogure ,
K. Ogua ,
M. Nakano  and
S. Yoshida
T. Kogure
Affiliation:
Department of Astronomy, Kyoto University, Sakyo-ku, Kyoto, Japan
K. Ogua
Affiliation:
Department of Natural Science, Kokugakuin University, Shibuya-ku, Tokyo, Japan
M. Nakano
Affiliation:
Department of Earth Science, Oita University, Oita, Japan
S. Yoshida
Affiliation:
Kiso Observatory, University of Tokyo, Kiso, Nagano, Japan
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Abstract

In this paper we present the results of spectroscopic observations for 34 emission-line stars (ELSs) in the Orion belt region, which were detected in an extensive survery. Spectral classification and the intensities of Hα and Hβ emission have revealed that the observed ELSs are probably T-Tauri type stars.

Type
Galactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 1 , 1991 , pp. 143
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Kogure, T., Yoshida, S., Wiramihardja, S. D., Nakano, M., Iwata, T. and Ogura, K., 1989, Publ. Astron. Soc. Japan, 41, 11.Google Scholar
Warren, W. H. and Hesser, J. E., 1977, Astrophys. J. Suppl. Ser., 34, 115.CrossRefGoogle Scholar
Wiramihardja, S. D., Kogure, T., Yoshida, S., Ogura, K. and Nakano, M., 1989, Publ. Astron. Soc. Japan, 41, 155.Google Scholar
Wiramihardja, S. D., Kogure, T., Yoshida, S., Nakano, M. and Ogura, K., 1990,(to be submitted).Google Scholar