Pulsation, Rotation and Mass Loss In Early-Type Stars

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Hardback. New. This volume discusses recent discoveries about O and B type stars. In particular, the reason for the increased mass loss of B type stars is considered, although a definite conclusion is not reached.

New. In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together for the first time in order to broaden our understanding of O and B stars. Thanks to advances in digital spectroscopy, new types of pulsating B stars have been discovered. The pulsations can be understood in terms of the recent revision… Read more about this item

Paperback / softback. New. In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together for the first time in order to broaden our understanding of O and B stars. The variability of radiatively-driven winds from O and B stars are likely related to the rotation of the star.

Paperback / softback. New. In this Symposium, researchers specializing in pulsation, rotation, magnetic fields and stellar winds are brought together for the first time in order to broaden our understanding of O and B stars. The variability of radiatively-driven winds from O and B stars are likely related to the rotation of the star.