Overview
This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models.
Full Product Details
Author: Icko Iben (University of Illinois, Urbana-Champaign)
Publisher: Cambridge University Press
Imprint: Cambridge University Press (Virtual Publishing)
ISBN: 9781139061223
ISBN 10: 1139061224
Publication Date: 05 December 2012
Audience:
Professional and scholarly
,
Professional and scholarly
,
Professional & Vocational
,
Professional & Vocational
Format: Undefined
Publisher's Status: Active
Availability: Available To Order
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Reviews
'This is a book by one of the most prolific researchers in the area of stellar evolution, and he has plenty to teach practitioners in the field … [the] style is always clear and straightforward … This is not a book for the faint-hearted, but it is certainly full of fascinating detail which will repay study by the active researcher … Iben has produced a classic monograph, which compares well with classics of the past, and I am pleased to have a copy.' The Observatory
'This is a book by one of the most prolific researchers in the area of stellar evolution, and he has plenty to teach practitioners in the field ... [the] style is always clear and straightforward ... This is not a book for the faint-hearted, but it is certainly full of fascinating detail which will repay study by the active researcher ... Iben has produced a classic monograph, which compares well with classics of the past, and I am pleased to have a copy.' The Observatory
Author Information
Icko Iben, Jr is Emeritus Distinguished Professor of Astronomy and Physics at the University of Illinois, Urbana-Champaign, where he also gained his MS and PhD degrees in Physics and where a Distinguished Lectureship in his name was established in 1998. He initiated his teaching career at Williams College (1958–1961), engaged in astrophysics research as a Senior Research Fellow at Cal Tech (1961–1964), and continued his teaching career at the Massachusetts Institute of Technology (1964–1972) and Illinois (1972–1999). He has held visiting Professorships at over a dozen institutions, including Harvard University, the University of California, Santa Cruz, the University of Bologna, Italy and Niigata University, Japan. He was elected to the US National Academy of Sciences in 1985 and his awards include the Russell Lectureship of the American Astronomical Society (1989), the George Darwin Lectureship (1984) and the Eddington Medal (1990) of the Royal Astronomical Society, and the Eminent Scientist Award of the Japan Society for the Promotion of Science (2003–2004).
