No CrossRef data available.
Article contents
INTER-DIVISION IV-V / WORKING GROUP ACTIVE B-TYPE STARS
Published online by Cambridge University Press: 01 December 2008
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Transactions T27A: Transactions IAU , December 2008 , pp. 242 - 244
- Copyright
- Copyright © International Astronomical Union 2009
References
Michel, E., Baglin, A., Auvergne, M., et al. 2006, in: Fridlund, M., Baglin, A., Lochard, J. & Conroy, L. (eds.), The CoRoT Mission, ESA-SP, 1306, 39Google Scholar
Okazaki, A. T., Owoki, S. P., & Stefl, S. (eds.) 2007, Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP-CS, 361Google Scholar
Peters, G. J., Gies, D. R., Grundstrom, E. D., & McSwain, M. V. 2008, ApJ, 686, 1280CrossRefGoogle Scholar
Walker, G. A. H., Kuschnig, R., Matthews, J. M., et al. 2005a, ApJ (Letters), 623, L145CrossRefGoogle Scholar
Walker, G. A. H., Kuschnig, R., Matthews, J. M. et al. 2005b, ApJ (Letters), 635, L77CrossRefGoogle Scholar
You have
Access