Convection In Astrophysics Iau S239

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Convection in Astrophysics (IAU S239)

Author: International Astronomical Union. Symposium
language: en
Publisher: Cambridge University Press
Release Date: 2007-06-07
Convection is ubiquitous throughout the Universe, and during the last three decades it has become the largest factor of uncertainty in theoretical models of stars and in the interpretation of observations on the basis of such models. Recently, numerical simulations of convection have dramatically improved in their potential to take into account both the large scale properties of the flow itself and the microphysical properties of the fluid. Observations have become accurate enough to provide stringent tests for both numerical simulations and models of convection. IAU S239 was held to further understanding of convection, bringing together leading researchers in solar and stellar physics, the physics of planets, and of accretion disks. With reviews, research contributions, and detailed recordings of plenary discussions, this book is a valuable resource for professional astronomers and graduate students interested in the interdisciplinary study of one of the key physical processes in astrophysics.
Proceedings of the Twenty Seventh General Assembly Rio de Janeiro 2009

Author: International Astronomical Union. General Assembly
language: en
Publisher: Cambridge University Press
Release Date: 2010-06-03
A complete record of the formal organisational and administrative proceedings of the XXVII General Assembly of the International Astronomical Union.
The Astrophysics of Emission-Line Stars

Author: Tomokazu Kogure
language: en
Publisher: Springer Science & Business Media
Release Date: 2010-05-05
Many types of stars show conspicuous emission lines in their optical spectra. These stars are broadly referred to as emission line stars. Emission line stars are attractive to many people because of their spectacular phenomena and their amazing varieties and variability. This book offers general information on emission line stars, starting from a brief introduction to stellar astrophysics, and then moving to a broad overview of emission line stars including early and late type stars as well as pre-main sequence stars. Detailed references and index are prepared for further reading. Tomokazu Kogure's email address: [email protected]