Compact Stellar X-ray Sources

Compact Stellar X-ray Sources PDF Author: Walter Lewin
Publisher: Cambridge University Press
ISBN: 1139451774
Category : Science
Languages : en
Pages : 667

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Book Description
X-ray astronomy is the prime available window on astrophysical compact objects: black holes, neutron stars and white dwarfs. In this book, prominent experts provide a comprehensive overview of the observations and astrophysics of these objects. This is a valuable reference for graduate students and active researchers.

Compact Stellar X-ray Sources

Compact Stellar X-ray Sources PDF Author: Walter Lewin
Publisher: Cambridge University Press
ISBN: 1139451774
Category : Science
Languages : en
Pages : 667

Get Book Here

Book Description
X-ray astronomy is the prime available window on astrophysical compact objects: black holes, neutron stars and white dwarfs. In this book, prominent experts provide a comprehensive overview of the observations and astrophysics of these objects. This is a valuable reference for graduate students and active researchers.

Accretion-driven Stellar X-ray Sources

Accretion-driven Stellar X-ray Sources PDF Author: Walter H. G. Lewin
Publisher:
ISBN: 9780521245210
Category : X-ray astronomy
Languages : en
Pages : 450

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Book Description


The Universe in X-Rays

The Universe in X-Rays PDF Author: Joachim E. Trümper
Publisher: Springer Science & Business Media
ISBN: 3540344128
Category : Science
Languages : en
Pages : 499

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Book Description
With contributions from leading scientists in the field, and edited by two of the most prominent astronomers of our time, this is a totally authoritative volume on X-ray astronomy that will be essential reading for everyone interested – from students to astrophysicists and physicists. All the aspects of this exciting area of study are covered, from astronomical instrumentation to extragalactic X-ray astronomy.

The Evolution of Galactic X-Ray Binaries

The Evolution of Galactic X-Ray Binaries PDF Author: J. Truemper
Publisher: Springer Science & Business Media
ISBN: 9400945949
Category : Science
Languages : en
Pages : 306

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Book Description
The idea to hold a conference on the Evolution of Close-Binary X-ray sources grew in the summer of 1984. At that time we were hoping that some new results would be harvested in the months to come which would stimulate further work. We were particularly looking towards the Euro pean X-ray Observatory, EXOSAT, for new contributions. How lucky we were; quite unexpected developments took place. Just prior to the conference, quasi-periodic oscillations (now known as QPO) were discovered in three bright low-mass X-ray binaries: GX 5-1, Sco X-1, and Cyg X-2. They played an important role at the meeting. The possibility that QPOs imply a neutron star magnetic dipole field, and a neutron star rotation period in the millisecond range, received a lot of attention. This is not surprising, as it lends support to the idea, suggested earlier, that the 6-msec binary radio pulsar PSR 1953+29 evolved from a stage in which it was a bright low-mass X-ray binary. There was special interest in the possibility of white dwarf collapse into a neutron star. This is a. particularly attractive way to form the bright low-mass X-ray binaries, often referred to as galactic bulge sources. It would allow for the possibility of a very young neutron star in a very old binary system. The relatively high magnetic fields that one could infer from QPO could then be explained.

X-ray Binaries

X-ray Binaries PDF Author: Walter H. G. Lewin
Publisher: Cambridge University Press
ISBN: 9780521599344
Category : Science
Languages : en
Pages : 688

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Book Description
X-ray binaries are some of the most varied and perplexing systems known to astronomers. The compact object which accretes mass from its companion star may be a white dwarf, neutron star, or black hole, whereas the donor star can be a 'normal' star or a white dwarf. The various combinations differ widely in their behaviour, and this timely volume provides a unique reference of our knowledge to date of all of them.Fifteen specially written chapters by a team of the world's foremost researchers in the field explore all aspects of the X-ray binaries. They cover the X-ray, ultraviolet, optical and radio properties of these violent systems and address key issues such as: how were these systems formed, and what will be their fate; how can we understand X-ray bursts, and how the quasi-periodic oscillations; what is the connection between millisecond radio pulsars and low-mass X-ray binaries; and how does the magnetic field of a neutron star decay?This long awaited review provides graduate students and researchers with the standard reference on X-ray binaries for many years to come.

Cataclysmic Variables and Low-Mass X-Ray Binaries

Cataclysmic Variables and Low-Mass X-Ray Binaries PDF Author: D.Q. Lamb
Publisher: Springer Science & Business Media
ISBN: 9400953194
Category : Science
Languages : en
Pages : 435

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Book Description
Since 1976 a meeting devoted to recent research on cataclysmic variables ("CV workshop") has been held annually somewhere in North America. Many of the meetings have been held - following a custom older than anyone reading this book - in locations with well-known recreational potential (e. g. Santa Cruz, CA; Boulder, CO). We thought hard about this custom while contemplating the possibility of organi zing a meeting in Massachusetts in the middle of winter. Nobody wants their meeting to go down in history as the smallest and dullest, and it ~ surely be the coldest. But on occasion, meeting organizers have defied custom and scheduled meetings for less~than-trendy places, and gotten away with it (Ur·bana, IL and Rochester, NY must be reckoned as examples of this). Encouraged by the spatial and temporal proximity of the American Astronomical Society meeting (Boston, January 9-12), we thought we might get away with it again, and so came to organize a meeting for January 12-15, 1983, in Cambridge, MA. There was another reason for a meeting at this time and place, we loftily proclaimed in early mailings. No one doubts that the CV's are closely related to the low-mass X-ray binaries ("LMXB' s"), in which the accreting star is usually, or perhaps always, more compact than a white dwarf. Many of the general characteristics of LMXB's sound pretty familiar to any student of CV's: orbital periods in the range 0.

Accretion Disks In Compact Stellar Systems

Accretion Disks In Compact Stellar Systems PDF Author: J Craig Wheeler
Publisher: World Scientific
ISBN: 9814504599
Category :
Languages : en
Pages : 440

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Book Description
Accretion disks in compact stellar systems containing white dwarfs, neutron stars or black holes are the principal laboratory for understanding the role of accretion disks in a wide variety of environments from proto-stars to quasars. Recent work on disk instabilities and dynamics has given a new theoretical framework with which to study accretion disks. Modeling of time-dependent phenomena provides new insight into the causes and interpretation of photometric and spectroscopic variability and new constraints on the fundamental physical problem — the origin of viscosity in accretion disks. This book contains expert reviews on the nature of limit cycle thermal instabilities and a variety of closely related topics from the theory of angular momentum transport to eclipse mapping of the disk structure. The result is a comprehensive contemporary survey of the structure and evolution of accretion disks in compact binary systems.

Cosmic Radiation in Contemporary Astrophysics

Cosmic Radiation in Contemporary Astrophysics PDF Author: M.M. Shapiro
Publisher: Springer Science & Business Media
ISBN: 9400954883
Category : Science
Languages : en
Pages : 270

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Book Description
This volume is the product of Lecturers in the fourth Course of the International School of Cosmic-Ray Astrophysics held at the Ettore Majorana Center in Erice, Sicily in November, 1984. The Course, devoted to "Cosmic Radiation in Contemporary Astrophysics," was concurrently a NATO-sponsored Advanced Study Institute (ASI). Cosmic-ray research is in a state of ferment. Precise measure ments - some made with instruments aboard sattelites and space probe- have been confronting models and theories with severe constraints. The observations of gamma-ray sources, notably Cyg X-3, at energies up to 16 10 eV, have opened up tantalizing possibilities of direct source iden tification. This ASI was devoted largely to interdisciplinary phenomena in cosmic-ray astrophysics whose understanding requires input from the other channels in astronomy. It explored the ways in which progress in cosmic-ray science might clarify phenomena observed in related disciplines. In trying to achieve this aim, we assembled a staff of lecturers representing various astrophysical specialties, such as radio astronomy, optical astronomy, X-ray astronomy, gamma-ray astronomy, and of course, particle astronomy (i.e., cosmic radiation). Students and other participants were likewise drawn from diverse backgrounds. Vigorous discussions enlivened almost every session.

X-Ray Binaries and Recycled Pulsars

X-Ray Binaries and Recycled Pulsars PDF Author: E.P. van den Heuvel
Publisher: Springer Science & Business Media
ISBN: 9401127042
Category : Science
Languages : en
Pages : 545

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Book Description
Proceedings of the NATO Advanced Research Workshop on X-Ray Binaries and the Formation of Binary and Millisecond Radio Pulsars, Santa Barbara, CA, U.S.A., Januari 21-25, 1991

High Energy Phenomena Around Collapsed Stars

High Energy Phenomena Around Collapsed Stars PDF Author: F. Pacini
Publisher: Springer Science & Business Media
ISBN: 9400938233
Category : Science
Languages : en
Pages : 370

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Book Description
Proceedings of the NATO Advanced Study Institute, Cargèse, Corsica, France, September 2-13, 1985