Lingua: Inglese
Editore: Springer-Verlag, New York, NY, 2002
ISBN 10: 3540435182 ISBN 13: 9783540435181
Cloth. Condizione: Fine. 241 pp. Tightly bound. Corners not bumped. Text is free of markings.
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Da: BargainBookStores, Grand Rapids, MI, U.S.A.
Hardback or Cased Book. Condizione: New. Relativistic Flows in Astrophysics. Book.
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Da: Antiquariat Bookfarm, Löbnitz, Germania
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Aggiungi al carrelloHardcover. XII, 241 p. Ex-library with stamp and library-signature. GOOD condition, some traces of use. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. C-05348 9783540435181 Sprache: Englisch Gewicht in Gramm: 550.
Da: Ria Christie Collections, Uxbridge, Regno Unito
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Da: Cherubz Books, York, Regno Unito
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Condizione: New. pp. 260.
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Lingua: Inglese
Editore: Springer Berlin Heidelberg 2010-02-19, 2010
ISBN 10: 3642078044 ISBN 13: 9783642078040
Da: Chiron Media, Wallingford, Regno Unito
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Aggiungi al carrelloPaperback. Condizione: New.
Lingua: Inglese
Editore: Springer Berlin Heidelberg, 2002
ISBN 10: 3540435182 ISBN 13: 9783540435181
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Aggiungi al carrelloGebunden. Condizione: New. Bridges the gap between standard textbook material and the research level1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ??ray, X-ray and UV continuum. Such activ.
Lingua: Inglese
Editore: Springer Berlin Heidelberg, 2010
ISBN 10: 3642078044 ISBN 13: 9783642078040
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 53,49
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - 1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ray, X-ray and UV continuum. Such active cores are the so-called Active Galactic Nuclei (AGN) and the radiation is commonly believed to be a result of gravitational energy released by matter spiraling around 9 a supermassive central black hole of about 10 M (see Fig. 1). Though the central engine which produces the enormous observed activity cannot be resolved observationally, a standard picture of an AGN has gradually emerged to explain the richness of the radiation spectra: - an accretion disk with radius from about 2 to 100 gravitational radii, R , g feeding the central black hole and emitting mainly in the UV and soft X-rays; - the broad line optically emitting clouds (BLR), which seem to be absent in 3 some sources (e. g. FRI, see hereafter) and extend up to a few 10 R from g the center.
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Aggiungi al carrelloGebunden. Condizione: Gut. Gebraucht - Gut Zustand: Gut, Mängelexemplar, XII, 241 p. About this book The topic of this book is the study of relativistic outflows such as those seen in gamma-ray bursts, microquasars and active galactic nuclei. The book starts with lectures on physical processes relevant to all astrophysical systems exhibiting relativistic flows. Further lectures concentrate on more specific aspects such as various mechanisms for particle acceleration and radiation from relativistically moving sources. This volume will thus be of interest to postgraduate students and nonspecialist researchers as a tutorial introduction to this subject as well as for the experienced researcher looking for a modern source of reference. Written for Researchers, postgraduate students.
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. Relativistic Flows in Astrophysics | A. W. Guthmann (u. a.) | Taschenbuch | xii | Englisch | 2010 | Springer | EAN 9783642078040 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Lingua: Inglese
Editore: Springer, Berlin, Springer Berlin Heidelberg, Springer Jul 2002, 2002
ISBN 10: 3540435182 ISBN 13: 9783540435181
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 76,95
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Aggiungi al carrelloBuch. Condizione: Neu. Neuware - 1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ray, X-ray and UV continuum. Such active cores are the so-called Active Galactic Nuclei (AGN) and the radiation is commonly believed to be a result of gravitational energy released by matter spiraling around 9 a supermassive central black hole of about 10 M (see Fig. 1). Though the central engine which produces the enormous observed activity cannot be resolved observationally, a standard picture of an AGN has gradually emerged to explain the richness of the radiation spectra: - an accretion disk with radius from about 2 to 100 gravitational radii, R , g feeding the central black hole and emitting mainly in the UV and soft X-rays; - the broad line optically emitting clouds (BLR), which seem to be absent in 3 some sources (e. g. FRI, see hereafter) and extend up to a few 10 R from g the center.
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Lingua: Inglese
Editore: Springer Berlin Heidelberg Dez 2010, 2010
ISBN 10: 3642078044 ISBN 13: 9783642078040
Da: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Germania
EUR 53,49
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ray, X-ray and UV continuum. Such active cores are the so-called Active Galactic Nuclei (AGN) and the radiation is commonly believed to be a result of gravitational energy released by matter spiraling around 9 a supermassive central black hole of about 10 M (see Fig. 1). Though the central engine which produces the enormous observed activity cannot be resolved observationally, a standard picture of an AGN has gradually emerged to explain the richness of the radiation spectra: - an accretion disk with radius from about 2 to 100 gravitational radii, R , g feeding the central black hole and emitting mainly in the UV and soft X-rays; - the broad line optically emitting clouds (BLR), which seem to be absent in 3 some sources (e. g. FRI, see hereafter) and extend up to a few 10 R from g the center. 260 pp. Englisch.
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Aggiungi al carrelloCondizione: New. Print on Demand pp. 260 Illus.
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Aggiungi al carrelloCondizione: New. Print on Demand pp. 260 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam.
Da: Biblios, Frankfurt am main, HESSE, Germania
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Aggiungi al carrelloCondizione: New. PRINT ON DEMAND pp. 260.
Lingua: Inglese
Editore: Springer Berlin Heidelberg, 2010
ISBN 10: 3642078044 ISBN 13: 9783642078040
Da: moluna, Greven, Germania
EUR 48,37
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Aggiungi al carrelloCondizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Bridges the gap between standard textbook material and the research level1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ??ray, X-ray and UV continuum. Such activ.
Lingua: Inglese
Editore: Springer Berlin Heidelberg, Springer Dez 2010, 2010
ISBN 10: 3642078044 ISBN 13: 9783642078040
Da: buchversandmimpf2000, Emtmannsberg, BAYE, Germania
EUR 53,49
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Aggiungi al carrelloTaschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -1. 1 Schematic Picture of AGN Some galaxies are known to emit radiation with extremely high luminosities from a rather small volume in the ray, X-ray and UV continuum. Such active cores are the so-called Active Galactic Nuclei (AGN) and the radiation is commonly believed to be a result of gravitational energy released by matter spiraling around 9 a supermassive central black hole of about 10 M (see Fig. 1). Though the central engine which produces the enormous observed activity cannot be resolved observationally, a standard picture of an AGN has gradually emerged to explain the richness of the radiation spectra: ¿ an accretion disk with radius from about 2 to 100 gravitational radii, R , g feeding the central black hole and emitting mainly in the UV and soft X-rays; ¿ the broad line optically emitting clouds (BLR), which seem to be absent in 3 some sources (e. g. FRI, see hereafter) and extend up to a few 10 R from g the center.Springer-Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 260 pp. Englisch.