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OverviewThis collection of papers describes the evolutionary path of stars of various masses. Observational data and theoretical modeling of the stellar atmosphere and the stellar interior and their interaction are presented, covering chemical peculiarities, mass loss, and explosion, all of which are strongly related to the hydrodynamic evolution of the interior. In particular the supernova SN 1987 A is discussed for the first time in detail, including the underground neutrino observations and the detection of X-rays from the supernova. The study of its progenitor, a B 3 supergiant, was related to the topics of chemical peculiarities and mass loss mechanisms and atmospheric models. The intended readers are professional astronomers and astrophysicists, as well as physicists. The book will also be an important source of information for graduate students. Full Product DetailsAuthor: Ken'ichi NomotoPublisher: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG Imprint: Springer-Verlag Berlin and Heidelberg GmbH & Co. K Edition: Softcover reprint of the original 1st ed. 1988 Volume: 305 Dimensions: Width: 17.00cm , Height: 2.50cm , Length: 24.40cm Weight: 0.834kg ISBN: 9783662137017ISBN 10: 3662137011 Pages: 468 Publication Date: 23 August 2014 Audience: Professional and scholarly , Professional & Vocational Format: Paperback Publisher's Status: Active Availability: Manufactured on demand ![]() We will order this item for you from a manufactured on demand supplier. Table of ContentsContents: Chemical Peculiarities as Probe of Stellar Evolution: Main-Sequence Stars. Cool Evolved Stars. Hot Evolved Stars.- Mass-Losing Stars In Different Stages of Evolution: Hot Stars. Cool Stars. Interacting Binaries.- Chemical and Dynamical Structures of Exploding Stars: Novae And Dwarf Novae. Supernovae.- Concluding Remarks.- List of Participants.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |