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A Spectroscopic Study of Be stars in the SMC Cluster NGC 330

Published online by Cambridge University Press:  12 April 2016

W. Hummel ,
W. Gässler ,
B. Muschielok ,
T. Szeifert ,
W. Seifert ,
I. Appenzeller  and
G. Rupprecht
W. Hummel
Affiliation:
Institut für AstronomieundAstrophysik und Universitätssternwarte München, Scheinerstr 1, D–81673 München, Germany
W. Gässler
Affiliation:
Institut für AstronomieundAstrophysik und Universitätssternwarte München, Scheinerstr 1, D–81673 München, Germany
B. Muschielok
Affiliation:
Institut für AstronomieundAstrophysik und Universitätssternwarte München, Scheinerstr 1, D–81673 München, Germany
T. Szeifert
Affiliation:
Institut für AstronomieundAstrophysik und Universitätssternwarte München, Scheinerstr 1, D–81673 München, Germany
W. Seifert
Affiliation:
Landessternwarte Heidelberg, Königsstuhl 12, D–69117 Heidelberg, Germany
I. Appenzeller
Affiliation:
Landessternwarte Heidelberg, Königsstuhl 12, D–69117 Heidelberg, Germany
G. Rupprecht
Affiliation:
ESO, Karl-Schwarzschildstr. 2, D–85745 Garching, Germany

Abstract

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We present low resolution spectroscopy of about 20 Be stars in the SMC cluster NGC 330 to confirm the high contents of Be stars in this cluster.

Type
1. Overview
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 79 - 82
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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