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Asymptotic Giant Branch Stars (Astronomy and Astrophysics Library)
 
 
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Asymptotic Giant Branch Stars (Astronomy and Astrophysics Library) [Hardcover]

Harm J. Habing (Editor), Hans Olofsson (Editor)

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Book Description

September 15, 2003 0387008802 978-0387008806 1

The underlying astrophysical mechanisms of the objects known as asymptotic giant branch stars - the structures that occur during the dramatic period prior to a star's death - is the main theme of this text. Over the past three decades, asymptotic giant branch stars have become a topic of their own, and the contributions to this volume all focus on these entities themselves, rather than their connections to other fields of astronomy. Among the many topics covered are new methods of high- quality infrared observation and the more detailed and realistic simulations made possible by increasingly fast computers. This collection should be useful to graduate students who work in the field, teachers who want to address the subject in their courses, and to astronomers from various backgrounds who are interested in the astrophysics of AGB stars.


Editorial Reviews

Review

From the reviews:

"AGB stars have red giants as progenitors, and are fated to become planetary nebulae and white dwarfs. This book comprises a set of papers dealing with all aspects of the physics of these stars. It is intended for a graduate study level … . the chapters which are designed to be self-standing do provide interesting discussions about theory and corroborative observations, and I think there is lot that can be gleaned … ." (Callum Potter, Journal of the British Astronomical Association, Vol. 114 (3), 2004)


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Inside This Book (learn more)
First Sentence:
"Asymptotic giant branch stars" developed into a broad, coherent field of research in the last quarter of the preceding century, but its roots go much deeper into the past and involve several serendipitous discoveries. Read the first page
Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
extrinsic stars, stellar envelope mass, barium stars, gas expansion velocity, full stellar models, red symbiotics, intershell convective zone, calculated column densities, radio line emission, equatorial density enhancement, strong maser emission, maser stars, overall spherical symmetry, hot bottom burning, yellow symbiotics, accreting star, fundamental mode pulsation, circumbinary disk, intershell region, barium systems, thermal pulse cycle, dust grain formation, first thermal pulse, carbon stars, envelope integrations
Key Phrases - Capitalized Phrases (CAPs): (learn more)
San Francisco, Magellanic Clouds, Kluwer Academic Publishers, Local Group, Cambridge University Press, Milky Way, Mira Ceti, New York, Large Magellanic Cloud, M-type Mira, Monte Carlo, Stellar Systems, Tracers of Stellar Populations, Van Eck, Acta Astronomica, Cyclical Variability, General Catalogue of Variable Stars, Magellanic Stream, Core He Flash, Editions Frontičres, Galactic Centre, González Delgado, Infrared Space Observatory, Mass Loss Mass, Ursa Minor
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