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Author: Michael M. Shara
Publisher:
ISBN:
Category : Science
Languages : en
Pages : 480
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Book Description
Annotation Thirty-one papers from the June 2000 New York conference discuss the following: hydrodynamics in stellar collisions and mergers; massive stars; collisions and merger products as star cluster populations; stellar collisions, pulsar planets, and helium white dwarf mergers; gigantic nuclei; general relativity, gravitational radiation, and gamma ray bursts; and, n-body simulations. There is no index. Annotation (c)2003 Book News, Inc., Portland, OR (booknews.com)
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Author: Michael M. Shara
Publisher:
ISBN:
Category : Science
Languages : en
Pages : 480
Get Book Here
Book Description
Annotation Thirty-one papers from the June 2000 New York conference discuss the following: hydrodynamics in stellar collisions and mergers; massive stars; collisions and merger products as star cluster populations; stellar collisions, pulsar planets, and helium white dwarf mergers; gigantic nuclei; general relativity, gravitational radiation, and gamma ray bursts; and, n-body simulations. There is no index. Annotation (c)2003 Book News, Inc., Portland, OR (booknews.com)
Author: Henri M. J. Boffin
Publisher: Springer
ISBN: 3662444348
Category : Science
Languages : en
Pages : 364
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Book Description
The existence of blue straggler stars, which appear younger, hotter, and more massive than their siblings, is at odds with a simple picture of stellar evolution. Such stars should have exhausted their nuclear fuel and evolved long ago to become cooling white dwarfs. They are found to exist in globular clusters, open clusters, dwarf spheroidal galaxies of the Local Group, OB associations and as field stars. This book summarises the many advances in observational and theoretical work dedicated to blue straggler stars. Carefully edited extended contributions by well-known experts in the field cover all the relevant aspects of blue straggler stars research: Observations of blue straggler stars in their various environments; Binary stars and formation channels; Dynamics of globular clusters; Interpretation of observational data and comparison with models. The book also offers an introductory chapter on stellar evolution written by the editors of the book.
Author: Sverre Aarseth
Publisher: Springer
ISBN: 1402084315
Category : Science
Languages : en
Pages : 405
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Book Description
Published under the auspices of the Royal Astronomical Society, this volume contains a set of extensive school tested lectures, with the aim to give a coherent and thorough background knowledge of the subject and to introduce the latest developments in N-body computational astrophysics. The topics cover a wide range from the classical few-body problem with discussions of resonance, chaos and stability to realistic modelling of star clusters as well as descriptions of codes, algorithms and special hardware for N-body simulations. This collection of topics, related to the gravitational N-body problem, will prove useful to both students and researchers in years to come. 1) Published under the auspices of the Royal Astronomical Society.
Author: Jean-René Roy
Publisher: Cambridge University Press
ISBN: 1108417019
Category : Nature
Languages : en
Pages : 311
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Book Description
A thought provoking study of the powerful impact of images in guiding astronomers' understanding of galaxies through time.
Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 980
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Book Description
Author:
Publisher:
ISBN:
Category : Power resources
Languages : en
Pages : 1472
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Book Description
Author: Francesca Matteucci
Publisher: Springer Science & Business Media
ISBN: 9401009384
Category : Science
Languages : en
Pages : 605
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Book Description
This review of the most up-to-date observational and theoretical information concerning the chemical evolution of the Milky Way compares the abundances derived from field stars and clusters, giving information on the abundances and dynamics of gas.
Author: Prasenjit Saha
Publisher: Oxford University Press
ISBN: 0198816464
Category : Science
Languages : en
Pages : 132
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Book Description
Working physicists, and especially astrophysicists, value a good `back-of-the-envelope' calculation, meaning a short, elegant computation or argument that starts from general principles and leads to an interesting result. This book guides students on how to understand astrophysics using general principles and concise calculations -- endeavouring to be elegant where possible and using short computer programs where necessary. The material proceeds in approximate historical order. The book begins with the Enlightenment-era insight that the orbits of the planets is easy, but the orbit of the Moon is a real headache, and continues to deterministic chaos. This is followed by a chapter on spacetime and black holes. Four chapters reveal how microphysics, especially quantum mechanics, allow us to understand how stars work. The last two chapters are about cosmology, bringing us to 21st-century developments on the microwave background and gravitational waves.
Author: John Archibald Wheeler
Publisher: W. W. Norton & Company
ISBN: 0393079481
Category : Biography & Autobiography
Languages : en
Pages : 388
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Book Description
Winner of the American Institute of Physics Science Writing Award "This delightful account is packed with insights…[Wheeler] is a consummately American physicist whose wide-ranging career spans much of a disturbing century." —Michael Riordan, New York Times Book Review He studied with Niels Bohr, taught Richard Feynman, and boned up on relativity with his friend and colleague Albert Einstein. John Archibald Wheeler's fascinating life brings us face to face with the central characters and discoveries of modern physics. He was the first American to learn of the discovery of nuclear fission, later coined the term "black hole," led a renaissance in gravitation physics, and helped to build Princeton University into a mecca for physicists. From nuclear physics, to quantum theory, to relativity and gravitation, Wheeler's work has set the trajectory of research for half a century. His career has brought him into contact with the most brilliant minds of his field; Fermi, Bethe, Rabi, Teller, Oppenheimer, and Wigner are among those he called colleagues and friends. In this rich autobiography, Wheeler reveals in fascinating detail the excitement of each discovery, the character of each colleague, and the underlying passion for knowledge that drives him still.
Author: Harm J. Habing
Publisher: Springer Science & Business Media
ISBN: 1475738765
Category : Science
Languages : en
Pages : 566
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Book Description
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.
