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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, T27A(4), p. 242-244, 2008

DOI: 10.1017/s1743921308025593

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Inter-Division Iv-V / Working Group Active B-Type Stars

Journal article published in 2008 by Juan Fabregat, Geraldine J. Peters, Stanley P. Owocki, Karen S. Bjorkman, Douglas R. Gies, Hubertus F. Henrichs, David A. McDavid, Coralie Neiner ORCID, Philippe Stee
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

The Working Group on Active B-type Stars (formerly known as the Working Group on Be Stars) was re-established under IAU Commission 29 at the IAU General Assembly in Montreal, Quebec (Canada) in 1979, and has been continuously active to the present. Its main goal is to promote and stimulate research and international collaboration on the field of the active early-type (OB) stars.

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