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Chinese and Japanese Participation in B/Be Star Campaigns1

Published online by Cambridge University Press:  12 April 2016

J. Hao
J. Hao*
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China National Astronomical Observatories, Chinese Academy of Sciences

Abstract

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In the early 1980’s, astronomers at the Beijing Astronomical Observatory (BAO) entered a collaboration in a long term photometric observing project on Be stars which included about 30 stars. For example, in 1983 the group at BAO organized a multi-site campaign to measure the short term variability of EW Lac, KX And, KY And, o And, and LQ And. In 1989, 48 Per was selected to be one of the targets of MuSiCoS campaign in which many stellar astronomers at the BAO participated. In 1991, the Be group at the BAO joined a campaign on the prototypical nonradially pulsating B star, 53 Per. In 1992, French & Chinese astronomers proposed a joint campaign on o And and EW Lac. Astronomers in Japan are also active in Be star campaigns and in 1993-5 they organized several campaigns on few well known Be stars (ζ Oph, EW Lac, ϒ Cas, λ Eri and 28 Cyg).

Type
5. Campaigns
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 364 - 371
Copyright
Copyright © Astronomical Society of the Pacific 2000

Footnotes

2

Visiting Astronomer, Beijing Astrophysics Center

1

supported by a grant of this colloquium and the Natural Science Foundation of China

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