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Inter-Division IV/V WG on Active OB Stars

Published online by Cambridge University Press:  01 December 2005

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Our group studies active early-type (OB) stars, with historical focus on classical Be stars, but extending in recent years to include Slowly Pulsating B-stars (SPB), Beta-Cephei stars, the strongly magnetic Bp stars, Luminous Blue Vairiable (LBV) stars, and B[e] stars. An overall goal is to understand the nature, origin, and consequences of this activity, in terms of both the stellar structure and evolution, as well as the distribution and dynamics of circumstellar material and mass outflows.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007