Overview
This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an ""asymptotic giant branch star"" or ""AGB star"". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called ""E-AGB""-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars.
Full Product Details
Author: Harm J. Habing ,
Hans Olofsson
Publisher: Springer-Verlag New York Inc.
Imprint: Springer-Verlag New York Inc.
Edition: Softcover reprint of the original 1st ed. 2004
Dimensions:
Width: 15.50cm
, Height: 2.90cm
, Length: 23.50cm
Weight: 0.872kg
ISBN: 9781441918437
ISBN 10: 1441918434
Pages: 562
Publication Date: 12 December 2011
Audience:
Professional and scholarly
,
Professional & Vocational
Format: Paperback
Publisher's Status: Active
Availability: Out of stock
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Reviews
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)
"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)"
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)
