Catalogue Of Cataclysmic Binaries Low Mass X Ray Binaries And Related Objects


Catalogue Of Cataclysmic Binaries Low Mass X Ray Binaries And Related Objects
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Catalogue Of Cataclysmic Binaries Low Mass X Ray Binaries And Related Objects


Catalogue Of Cataclysmic Binaries Low Mass X Ray Binaries And Related Objects
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Author : Hans Ritter
language : en
Publisher:
Release Date : 1983

Catalogue Of Cataclysmic Binaries Low Mass X Ray Binaries And Related Objects written by Hans Ritter and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1983 with Double stars categories.




Cataclysmic Variables And Low Mass X Ray Binaries


Cataclysmic Variables And Low Mass X Ray Binaries
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Author : D.Q. Lamb
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06

Cataclysmic Variables And Low Mass X Ray Binaries written by D.Q. Lamb and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.


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.



Highly Evolved Close Binary Stars


Highly Evolved Close Binary Stars
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Author : Anatoliĭ Mikhaĭlovich Cherepashchuk
language : en
Publisher: Taylor & Francis
Release Date : 1996

Highly Evolved Close Binary Stars written by Anatoliĭ Mikhaĭlovich Cherepashchuk and has been published by Taylor & Francis this book supported file pdf, txt, epub, kindle and other format this book has been release on 1996 with Science categories.




The Evolution Of Galactic X Ray Binaries


The Evolution Of Galactic X Ray Binaries
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Author : J. Truemper
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06

The Evolution Of Galactic X Ray Binaries written by J. Truemper and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.


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.



Literature 1984 Part 2


Literature 1984 Part 2
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Author : S. Böhme
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-04-17

Literature 1984 Part 2 written by S. Böhme and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-04-17 with Science categories.




Cataclysmic Variables And Related Objects Pp I Xc 1 342


Cataclysmic Variables And Related Objects Pp I Xc 1 342
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Author : Margherita Hack
language : en
Publisher:
Release Date : 1993

Cataclysmic Variables And Related Objects Pp I Xc 1 342 written by Margherita Hack and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1993 with Cataclysmic variable stars categories.




X Ray Binaries


X Ray Binaries
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Author : Walter H. G. Lewin
language : en
Publisher: Cambridge University Press
Release Date : 1997-01-16

X Ray Binaries written by Walter H. G. Lewin and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 1997-01-16 with Science categories.


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.



Literature 1987 Part 2


Literature 1987 Part 2
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Author : U. Esser
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-11-11

Literature 1987 Part 2 written by U. Esser and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-11-11 with Science categories.


Astronomy and Astrophysics Abstracts aims to present a comprehensive documen tation of the literature concerning all aspects of astronomy, astrophysies, and their border fields. It is devoted to the recording, summarizing, and indexing of the relevant publications throughout the world. Astronomy and Astrophysics Abstracts is prepared by a special department of the Astronomisches Rechen-Institut under the auspices of the International Astronomical Union. Volume 44 records literature published in 1987 and received before February 15, 1988. Some older documents which we received late and which are not surveyed in earlier volumes are inc1uded too. We acknowledge with thanks contributions of our colleagues all over the world. We also express our gratitude to all organiza tions, observatories, and publishers which provide us with complimentary copies of their publications. Dr. Siegfried Böhme retired from his duties as co-editor of Astronomy and Astro physics Abstracts on December 31, 1987. Since 1950 he partieipated in the biblio graphie work of the institute. He served as a reviewer for the Astronomischer Jahresbericht and became one of the editors of Astronomy and Astrophysics Ab stracts in 1969. After his retirement in 1975 he took care of, particularly, the Russian literature on a voluntary basis for 12 years. It is a pleasure to thank Siegfried Böhme for his valuable contributions. Starting with Volume 33, all the recording, correction, and data processing work was done by means of computers. The recording was done by our technical staff members Ms. Helga Ballmann, Ms. Christiane Jehn, Ms. Monika Kohl, Ms.



Cataclysmic Variables Recent Multi Frequency Observations And Theoretical Developments


Cataclysmic Variables Recent Multi Frequency Observations And Theoretical Developments
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Author : H. Drechsel
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06

Cataclysmic Variables Recent Multi Frequency Observations And Theoretical Developments written by H. Drechsel and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.


Recent advances in observational and theoretical efforts in understanding the nature of cataclysmic variables had reached such maturity that there existed a strong, shared feeling among the workers in this field that an international colloquium sponsored by the International Astronomical Union would be timely. To be more specific, this was due primarily to the accumulation of the new data from satellite observatories, such as the International Ultraviolet Observatory (IUE) and EXOSAT, as well as ground-based optical and radio telescopes, and the advances in modeling the putative accretion disks and the thermo-nuclear run-away phenomena in the vinicity of the white dwarf stars in cataclysmic variables. A series of workshops on this subject held in North America over the past several years and that held in Europe in 1985 had all contributed to the advances in our knowledge that led to IAU Colloguium No. 93, held in Bamberg from the 16th to 19th of June 1986. In all, 157 astronomers from 27 countries participated in this conference. Judging from the papers presented, both invited and contributed, and from the enthusiasm seen in discussions, the meeting was indeed a success.



A Reference Catalogue And Atlas Of Galactic Novae


A Reference Catalogue And Atlas Of Galactic Novae
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Author : Hilmar W. Duerbeck
language : en
Publisher: Springer Science & Business Media
Release Date : 2013-03-09

A Reference Catalogue And Atlas Of Galactic Novae written by Hilmar W. Duerbeck and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2013-03-09 with Science categories.


4. Census of the Catalogue The catalogue contains information on 277 objects. 137 (50%) of them are stars whose outburst spectra or unambiguous mInImUm characteristics classify them as novae beyond doubt. 123 of them could be identified at minimum. 78 (28 %) are stars with amplitudes and light curve forms which makes nova classifi cation likely. 60 of them could be identified at minimum. Thus, 78 % ofthe objects in this catalogue are confirmed and suspected classical novae. 16 (6%) have properties compatible with both novae and related objects. 15 are identified at minimum. Furthermore, the catalogue and atlas contains data on 12 (4 %) dwarf novae of long cycle length or suspected dwarf novae for which only one outburst has been observed. Examples are WZ Sge and CI Gern. 6 (2%) recurrent novae or suspected recurrent novae are listed. Examples are T CrB and AS Psc. 6 (2%) X-ray novae are listed. Examples are V616 Mon and KY TrA. 6 (2%) symbiotic stars and symbiotic novae are listed. Examples are RT Ser and V352 Aql. 11 (4 %) Mira stars or suspected Mira stars, which at some time were believed to be novae, are listed. Examples are V607 Aql and V927 Sgr.