Hostname: page-component-77c89778f8-fv566 Total loading time: 0 Render date: 2024-07-16T11:51:11.423Z Has data issue: false hasContentIssue false

Emission Line Variability of DR Tau

Published online by Cambridge University Press:  25 April 2016

Syuzo Isobe
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, Japan
Yuji Norimoto
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, Japan
Hajime Kawakami
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo, Japan

Abstract

This paper presents results of CCD observations of DR Tau which show emission line variability.

Type
Galactic and Stellar
Copyright
Copyright © Astronomical Society of Australia 1991

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Aiad, A., Appenzeller, I., Beitout, C., Isobe, S., Shimizu, M., Stahl, O., Walker, M. F. and Wolf, B., 1984, Astron. Astrophys., 130, 67.Google Scholar
Appenzeller, I., Jankovics, I. and Jetter, R., 1986, Astron. Astrophys. Suppl. Ser., 64, 65.Google Scholar
Isobe, S., Norimoto, Y. and Kitamura, T., 1988, Publ. Astron. Soc. Japan, 40, 89.Google Scholar
Joy, A. H., 1949, Astrophys. J., 110, 424.CrossRefGoogle Scholar