Describes how stars respond to microscopic physics in the advanced stages of their evolution with many numerical examples and illustrations.
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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 the California Institute of Technology (1961–1964), and continued his teaching career at the Massachusetts Institute of Technology (1964–1972) and the University of 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).
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Da: HPB-Red, Dallas, TX, U.S.A.
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Da: Prior Books Ltd, Cheltenham, Regno Unito
Hardcover. Condizione: Like New. First Edition. A firm and square hardback with sharp corners and strong joints, just showing a few very minor cosmetic rubs. Hence a non-text page has a small 'damaged' stamp. Despite such this book is actually in nearly new condition and appears unread. Thus the contents are crisp, fresh and tight; no pen-marks. Now offered for sale at a very sensible price. Codice articolo 211825
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Da: moluna, Greven, Germania
Gebunden. Condizione: New. This text explains the microscopic physics operating in stars in advanced stages of their evolution, using numerical examples and illustrations to demonstrate how they respond. The volume allows senior graduate students and researchers who have mastered the. Codice articolo 595312029
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Condizione: New. pp. 616. Codice articolo 2642163149
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Da: CitiRetail, Stevenage, Regno Unito
Hardcover. Condizione: new. Hardcover. This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and helium burning) and through the final cooling white dwarf phase. A massive model is carried from the core helium-burning phase through core and shell carbon-burning phases. Gravothermal responses to nuclear reaction-induced transformations and energy loss from the surface are described in detail. Written for senior graduate students and researchers who have mastered the principles of stellar evolution, as developed in the first volume of Stellar Evolution Physics, sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level. This text explains the microscopic physics operating in stars in advanced stages of their evolution, using numerical examples and illustrations to demonstrate how they respond. The volume allows senior graduate students and researchers who have mastered the principles of stellar evolution to engage in model construction on a professional level. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. Codice articolo 9781107016576
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