Short-period binary stars : observations, analyses, and results

Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. These objects represent stages of evolution of binary stars, and...

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Other Authors: Milone, Eugene F.
Format: Book
Language:English
Published: Springer 2017
Subjects:
520
Online Access:http://repository.vnu.edu.vn/handle/VNU_123/29840
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Institution: Vietnam National University, Hanoi
Language: English
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spelling oai:112.137.131.14:VNU_123-298402020-10-14T02:24:46Z Short-period binary stars : observations, analyses, and results Milone, Eugene F. Leahy, Denis A. Hobill, David W. Double stars Astronomy 520 Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. These objects represent stages of evolution of binary stars, and their degrees of separation provide critical clues to how their evolutionary paths differ from that of single stars. The widest and least distorted systems provide astronomers with the essential precise data needed to study all stars: mass and radius. The interactions of binary star components, on the other hand, provide a natural laboratory to observe how the matter in these stars behaves under different and often varying physical conditions. Thus, cataclysmic variables with and without overpoweringly strong magnetic fields, and stars with densities from that found in the Sun to the degenerate matter of white dwarfs and the ultra-compact states of neutron stars and black holes are all discussed. The extensive index permits cross-referencing. The objects being discussed are carefully defined in each section and the contributions are organized according to the compactness of the binaries that are treated. Some treatments are of individual objects; others are more general. The observational techniques that are used by the contributors to throw light on these objects include gravitational wave investigations, X-ray, radio, infrared, and optical astronomy; and the ways in which these objects are analyzed is also discussed. Among the specific objects reported is the Double Pulsar, highlighting what observations of this object tell us about fundamental physics. The level of the book is appropriate for both professional astronomers in the field as well as people interested in other fields and dedicated amateur astronomers. 2017-04-17T07:30:07Z 2017-04-17T07:30:07Z 2008 Book 978-1-4020-6543-9 http://repository.vnu.edu.vn/handle/VNU_123/29840 en © 2008 Springer Science+Business Media B.V. 277 p. application/pdf Springer
institution Vietnam National University, Hanoi
building VNU Library & Information Center
country Vietnam
collection VNU Digital Repository
language English
topic Double stars
Astronomy
520
spellingShingle Double stars
Astronomy
520
Short-period binary stars : observations, analyses, and results
description Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. These objects represent stages of evolution of binary stars, and their degrees of separation provide critical clues to how their evolutionary paths differ from that of single stars. The widest and least distorted systems provide astronomers with the essential precise data needed to study all stars: mass and radius. The interactions of binary star components, on the other hand, provide a natural laboratory to observe how the matter in these stars behaves under different and often varying physical conditions. Thus, cataclysmic variables with and without overpoweringly strong magnetic fields, and stars with densities from that found in the Sun to the degenerate matter of white dwarfs and the ultra-compact states of neutron stars and black holes are all discussed. The extensive index permits cross-referencing. The objects being discussed are carefully defined in each section and the contributions are organized according to the compactness of the binaries that are treated. Some treatments are of individual objects; others are more general. The observational techniques that are used by the contributors to throw light on these objects include gravitational wave investigations, X-ray, radio, infrared, and optical astronomy; and the ways in which these objects are analyzed is also discussed. Among the specific objects reported is the Double Pulsar, highlighting what observations of this object tell us about fundamental physics. The level of the book is appropriate for both professional astronomers in the field as well as people interested in other fields and dedicated amateur astronomers.
author2 Milone, Eugene F.
author_facet Milone, Eugene F.
format Book
title Short-period binary stars : observations, analyses, and results
title_short Short-period binary stars : observations, analyses, and results
title_full Short-period binary stars : observations, analyses, and results
title_fullStr Short-period binary stars : observations, analyses, and results
title_full_unstemmed Short-period binary stars : observations, analyses, and results
title_sort short-period binary stars : observations, analyses, and results
publisher Springer
publishDate 2017
url http://repository.vnu.edu.vn/handle/VNU_123/29840
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