Active OB stars: structure, evolution, mass loss, and critical limits
Contributed Papers
Active OB Stars - an introduction
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- 12 July 2011, pp. 1-13
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Rapid rotation and mixing in active OB stars – Physical processes
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- 12 July 2011, pp. 14-25
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Mixing of CNO-cycled matter in pulsationally and magnetically active massive stars
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- 12 July 2011, pp. 26-31
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3D MHD simulations of subsurface convection in OB stars
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- 12 July 2011, pp. 32-37
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Rotation rates of massive stars in the Magellanic Clouds
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- 12 July 2011, pp. 38-43
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Interferometric studies of rapid rotators
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- 12 July 2011, pp. 44-55
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Effects of fast rotation on the wind of Luminous Blue Variables
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- 12 July 2011, pp. 56-61
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Massive stellar models: rotational evolution, metallicity effects
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- 12 July 2011, pp. 62-72
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Testing models of rotating stars
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- 12 July 2011, pp. 73-78
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Discussion – Rapid rotation and mixing in active OB stars
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- 12 July 2011, pp. 79-82
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Radiation driven winds with rotation: the oblate finite disc correction factor
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- 12 July 2011, pp. 83-84
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Where do Be stars stand in the picture of rotational mixing?
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- 12 July 2011, pp. 85-86
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About the Luminous Blue Variable He3-519
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- 12 July 2011, pp. 87-88
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Results from a recent stellar rotation census of B stars
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- 12 July 2011, pp. 89-90
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Mass and angular momentum loss of fast rotating stars via decretion disks
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- 12 July 2011, pp. 91-92
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Mass loss in 2D rotating stellar models
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- 12 July 2011, pp. 93-94
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Models of classical Be stars with gravity darkening
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- 12 July 2011, pp. 95-96
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Mixing in two magnetic OB stars discovered by the MiMeS collaboration
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- 12 July 2011, pp. 97-98
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Evolutionary effects of stellar rotation of massive stars in their pre-supernova environments
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- 12 July 2011, pp. 99-100
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The Nitrogen Abundance in Be Stars Determined from UV Spectra
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- 12 July 2011, pp. 101-102
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