Evolutionary Processes In Interacting Binary Stars
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Author |
: Y. Kondo |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 570 |
Release |
: 1992-06-30 |
ISBN-10 |
: 0792317319 |
ISBN-13 |
: 9780792317319 |
Rating |
: 4/5 (19 Downloads) |
Synopsis Evolutionary Processes in Interacting Binary Stars by : Y. Kondo
This book contains the proceedings of IAU Symposium No. 151 `Evolutionary Processes in Interacting Binary Stars,' which was held from 5 to 9 August 1991 in Cordóba, Argentina. The primary aim of this conference was to review and evaluate our current understanding of the evolutionary processes in wide variety of interacting binary stars from their births to their deaths. Subjects included the formation of binaries, mass flow and transfer, accretion processes, and binaries with collapsed components, such as novae, X-ray binaries and binary pulsars. As the field covered is both broad and diverse, there were in all thirty-seven invited talks; sixty-two contributed papers were also presented. In addition, these proceedings contain comments from a panel discussion of the major unsolved problems of interacting binary stars.
Author |
: Peter Eggleton |
Publisher |
: Cambridge University Press |
Total Pages |
: 331 |
Release |
: 2006-07-20 |
ISBN-10 |
: 9781139456951 |
ISBN-13 |
: 1139456954 |
Rating |
: 4/5 (51 Downloads) |
Synopsis Evolutionary Processes in Binary and Multiple Stars by : Peter Eggleton
Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.
Author |
: Y. Kondo |
Publisher |
: Springer |
Total Pages |
: 0 |
Release |
: 1992-07-14 |
ISBN-10 |
: 9401125422 |
ISBN-13 |
: 9789401125420 |
Rating |
: 4/5 (22 Downloads) |
Synopsis Evolutionary Processes in Interacting Binary Stars by : Y. Kondo
This book contains the proceedings of IAU Symposium No. 151 `Evolutionary Processes in Interacting Binary Stars,' which was held from 5 to 9 August 1991 in Cordóba, Argentina. The primary aim of this conference was to review and evaluate our current understanding of the evolutionary processes in wide variety of interacting binary stars from their births to their deaths. Subjects included the formation of binaries, mass flow and transfer, accretion processes, and binaries with collapsed components, such as novae, X-ray binaries and binary pulsars. As the field covered is both broad and diverse, there were in all thirty-seven invited talks; sixty-two contributed papers were also presented. In addition, these proceedings contain comments from a panel discussion of the major unsolved problems of interacting binary stars.
Author |
: Peter Eggleton |
Publisher |
: |
Total Pages |
: 332 |
Release |
: 2006 |
ISBN-10 |
: 0511225725 |
ISBN-13 |
: 9780511225727 |
Rating |
: 4/5 (25 Downloads) |
Synopsis Evolutionary Processes in Binary and Multiple Stars. Cambridge Astrophysics Series by : Peter Eggleton
Author |
: R.A. Wijers |
Publisher |
: Springer |
Total Pages |
: 412 |
Release |
: 2011-09-26 |
ISBN-10 |
: 9401072493 |
ISBN-13 |
: 9789401072496 |
Rating |
: 4/5 (93 Downloads) |
Synopsis Evolutionary Processes in Binary Stars by : R.A. Wijers
7 Hydrodynamic Instabilities in Close Binary Systems (Frederic A. Rasio) 121 7. 1 Introduction. . . . . . . . . . . . . . . . . . . . . . . . 121 7. 1. 1 The stability of self-gravitating fluid equilibria 121 7. 1. 2 Astrophysical motivation . 123 7. 1. 3 Common envelope systems 125 7. 2 Dynamical instabilities. . . . . . . 126 7. 2. 1 Physical mechanism . . . . 126 7. 2. 2 Application to coalescing neutron star binaries 127 7. 3 Secular instabilities. . . . . . . . . . . 130 7. 3. 1 Physical mechanism . . . . . . 130 7. 3. 2 Application to contact binaries 133 8 Common Envelope Evolution in Binary Systems (Mario Livio) 141 8. 1 Introduction. . . . . . . . . . . . . . . . . . . . 141 8. 2 The entrance into the common envelope phase . . . . . 142 8. 3 The outcome of the CE phase. . . . . . . . . . . . . . . 145 8. 4 How close can we get to observing the common envelope Phase? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 146 8. 4. 1 How can PNe with binary nuclei be used to constrain CE physics . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 8. 4. 2 How can nova systems be used to constrain CE physics 148 8. 4. 3 Other tests of common envelope evolution 150 8. 5 Conclusions . . . . . . . . . . . . . . . . . . . . . . . 151 9 Structure and Evolution of Massive Close Binaries (Dany Vanbeveren) 155 9. 1 Introduction. . . . . . . . . . . . . . . . . . 155 9. 2 Definitions. . . . . . . . . . . . . . . . . . . 156 9. 3 Intermediate mass and massive single stars 156 9. 3. 1 Observations . . . . . . . . . . . . . 156 9. 3. 2 Stellar structure equations for non-rotating IMS's and MS's 160 9. 3. 3 Evolutionary computations of non-rotating IMS's and MS's 162 9. 3. 4 Overall comparison with observations '" 163 9. 3. 5 The role of rotation in single star evolution . . .
Author |
: Matthew Benacquista |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 262 |
Release |
: 2012-11-28 |
ISBN-10 |
: 9781441999917 |
ISBN-13 |
: 1441999914 |
Rating |
: 4/5 (17 Downloads) |
Synopsis An Introduction to the Evolution of Single and Binary Stars by : Matthew Benacquista
An Introduction to the Evolution of Single and Binary Stars provides physicists with an understanding of binary and single star evolution, beginning with a background and introduction of basic astronomical concepts. Although a general treatment of stellar structure and evolution is included, the text stresses the physical processes that lead to stellar mass compact object binaries that may be sources of observable gravitational radiation. Basic concepts of astronomy, stellar structure and atmospheres, single star evolution, binary systems and mass transfer, compact objects, and dynamical systems are covered in the text. Readers will understand the astrophysics behind the populations of compact object binary systems and have sufficient background to delve deeper into specific areas of interest. In addition, derivations of important concepts and worked examples are included. No previous knowledge of astronomy is assumed, although a familiarity with undergraduate quantum mechanics, classical mechanics, and thermodynamics is beneficial.
Author |
: P.P. Eggleton |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 418 |
Release |
: 2012-12-06 |
ISBN-10 |
: 9789400953376 |
ISBN-13 |
: 9400953372 |
Rating |
: 4/5 (76 Downloads) |
Synopsis Interacting Binaries by : P.P. Eggleton
Peter P. Eggleton and James E. Pringle Institute of Astronomy Madingley Road Cambridge England The 1970's can be described, in retrospect, as the "Decade of the Close Binary". Exciting observations with new technology, combined with classical work, both observational and theoretical, convinced the astronomical world that binary interaction of various kinds is not only interesting but common. Indeed, by 1975 almost anything unusual had a good chance of being interpreted as due to binary interaction. But astronomers are seldom overwhelmed by speculation, even their own, and solid observational work has confirmed or refuted such speculation, without regard to its plausibility. For instance, binarity has been found where it was perhaps least expected, in Barium stars, and refuted where it could most reasonably be expected, in Wolf-Rayets. Unfortunately, many other classes of potential binaries remain without the clearest evidence of binarity, for instance Be stars, symbiotics and blue stragglers. This Advanced Study Institute was held to commemorate John Whelan (1945-1981), whose scientific career, sadly cut short in its prime, did much to further the careful study, theoretical and observational, of close binaries, as well as to encourage the spirit of international friendship and collaboration. His own interests covered a greater field, but "Interacting Binaries" seemed a reasonable restriction. We publish here 15 review talks, which still do not cover the whole topic, although they range widely.
Author |
: Giacomo Beccari |
Publisher |
: Cambridge University Press |
Total Pages |
: 359 |
Release |
: 2019-04-18 |
ISBN-10 |
: 9781108681940 |
ISBN-13 |
: 1108681948 |
Rating |
: 4/5 (40 Downloads) |
Synopsis The Impact of Binary Stars on Stellar Evolution by : Giacomo Beccari
Stars are mostly found in binary and multiple systems, with at least 50% of all solar-like stars having companions; this fraction approaches 100% for the most massive stars. A large proportion of these systems interact and alter the structure and evolution of their components, leading to exotic objects such as Algol variables, blue stragglers and other chemically peculiar stars, but also to phenomena such as non-spherical planetary nebulae, supernovae and gamma-ray bursts. While it is understood that binaries play a critical role in the Initial Mass Function, the interactions among binary systems significantly affect the dynamical evolution of stellar clusters and galaxies. This interdisciplinary volume presents results from state-of-the-art models and observations aimed at studying the impact of binaries on stellar evolution in resolved and unresolved populations. Serving as a bridge between observational and theoretical astronomy, it is a comprehensive review for researchers and advanced students of astrophysics.
Author |
: Astronomisches Recheninstitut |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 1456 |
Release |
: 2013-11-11 |
ISBN-10 |
: 9783662123799 |
ISBN-13 |
: 3662123797 |
Rating |
: 4/5 (99 Downloads) |
Synopsis Literature 1992, Part 1 by : Astronomisches Recheninstitut
"Astronomy and Astrophysics Abstracts" appearing twice a year has become oneof the fundamental publications in the fields of astronomy, astrophysics andneighbouring sciences. It is the most important English-language abstracting journal in the mentioned branches. The abstracts are classified under more than a hundred subject categories, thus permitting a quick survey of the whole extended material. The AAA is a valuable and important publication for all students and scientists working in the fields of astronomy and related sciences. As such it represents a necessary ingredient of any astronomical library all over the world.
Author |
: Thomas M Tauris |
Publisher |
: Princeton University Press |
Total Pages |
: 864 |
Release |
: 2023-06-20 |
ISBN-10 |
: 9780691179087 |
ISBN-13 |
: 0691179085 |
Rating |
: 4/5 (87 Downloads) |
Synopsis Physics of Binary Star Evolution by : Thomas M Tauris
A graduate-level textbook on the astrophysics of binary star systems and their evolution Physics of Binary Star Evolution is an up-to-date textbook on the astrophysics and evolution of binary star systems. Theoretical astrophysicists Thomas Tauris and Edward van den Heuvel cover a wide range of phenomena and processes, including mass transfer and ejection, common envelopes, novae and supernovae, X-ray binaries, millisecond radio pulsars, and gravitational wave (GW) sources, and their links to stellar evolution. The authors walk through the observed properties and evolution of different types of binaries, with special emphasis on those containing compact objects (neutron stars, black holes, and white dwarfs). Attention is given to the formation mechanisms of GW sources—merging double neutron stars and black holes as well as ultra-compact GW binaries hosting white dwarfs—and to the progenitors of these sources and how they are observed with radio telescopes, X-ray satellites, and GW detectors (LIGO, Virgo, KAGRA, Einstein Telescope, Cosmic Explorer, and LISA). Supported by illustrations, equations, and exercises, Physics of Binary Star Evolution combines theory and observations to guide readers through the wonders of a field that will play a central role in modern astrophysics for decades to come. 465 equations, 47 tables, and 350+ figures More than 80 exercises (analytical, numerical, and computational) Over 2,500 extensive, up-to-date references