Compartir
Active ob Stars (Iau S272): Structure, Evolution, Mass-Loss, and Critical Limits (Proceedings of the International Astronomical Union Symposia and Colloquia) (en Inglés)
Neiner; Wade; Meynet (Autor)
·
Cambridge University Press
· Tapa Dura
Active ob Stars (Iau S272): Structure, Evolution, Mass-Loss, and Critical Limits (Proceedings of the International Astronomical Union Symposia and Colloquia) (en Inglés) - Neiner; Wade; Meynet
$ 121.310
$ 202.180
Ahorras: $ 80.870
Elige la lista en la que quieres agregar tu producto o crea una nueva lista
✓ Producto agregado correctamente a la lista de deseos.
Ir a Mis Listas
Origen: Estados Unidos
(Costos de importación incluídos en el precio)
Se enviará desde nuestra bodega entre el
Jueves 30 de Mayo y el
Martes 11 de Junio.
Lo recibirás en cualquier lugar de Chile entre 1 y 3 días hábiles luego del envío.
Reseña del libro "Active ob Stars (Iau S272): Structure, Evolution, Mass-Loss, and Critical Limits (Proceedings of the International Astronomical Union Symposia and Colloquia) (en Inglés)"
IAU Symposium 272 presents an overview of the latest research into active OB stars. These massive, volatile objects serve as test beds for extreme conditions, and research into them has entered a new era with the advent of new space and round-based instrumentation. In this volume, renowned experts discuss the cutting-edge observations, state-of-the-art modeling and recently developed techniques such as asteroseismology, interferometry and spectropolarimetry that have improved our understanding of these extreme objects. Asteroseismology allows us to infer the internal structure of massive stars and their rotation; high-resolution spectropolarimetry provides clues about magnetic fields and the confinement of their circumstellar environments; and interferometry probes the shape of these environments and investigates differential rotation. Written for researchers and graduate students, this volume will appeal to all those interested in extreme physical processes as tools to study structure evolution and mass loss of active OB stars.