2010, ISBN: 3838391136

[EAN: 9783838391137], Neubuch, [PU: LAP Lambert Acad. Publ. Aug 2010], This item is printed on demand - Print on Demand Neuware - The calculation of (general-relativistic) geodesics in the vicinity of spinning Black Holes (BHs), i.e. in Kerr metric, allows to interpret some features detected in the X-ray spectra of many Active Galactic Nuclei (AGN) and galactic BH candidates, like the typical asymmetric profile of the iron K line. Our assumptions (Kerr metric, disc illumination from a central source) may also yield a simple explanation of the K line equivalent width measured in some sources. In order to allow comparison with the data, we developed a computational tool aimed to fit the observed spectral features - including the disc-reflected continuum - on the base of fully relativistic models. The research we present here was performed under the supervision of V. Karas (AV R, Prague), E. Massaro (Uni1, Rome), G. Matt (Uni3, Rome), J. Miller (SISSA, Trieste). The present results were submitted as a Dissertation for the degree of Doctor Philosophiae at SISSA (Trieste), in October 2000. 164 pp. Englisch

2000, ISBN: 9783838391137

Paperback, [PU: LAP Lambert Academic Publishing], The calculation of (general-relativistic) geodesics in the vicinity of spinning Black Holes (BHs), i.e. in Kerr metric, allows to interpret some features detected in the X-ray spectra of many Active Galactic Nuclei (AGN) and galactic BH candidates, like the typical asymmetric profile of the iron K line. Our assumptions (Kerr metric, disc illumination from a central source) may also yield a simple explanation of the K line equivalent width measured in some sources. In order to allow comparison with the data, we developed a computational tool aimed to fit the observed spectral features - including the disc-reflected continuum - on the base of fully relativistic models. The research we present here was performed under the supervision of V. Karas (AV R, Prague), E. Massaro (Uni1, Rome), G. Matt (Uni3, Rome), J. Miller (SISSA, Trieste). The present results were submitted as a Dissertation for the degree of Doctor Philosophiae at SISSA (Trieste), in October 2000., Astronomy, Space & Time

2000, ISBN: 9783838391137

The calculation of (general-relativistic) geodesics in the vicinity of spinning Black Holes (BHs), i.e. in Kerr metric, allows to interpret some features detected in the X-ray spectra of many Active Galactic Nuclei (AGN) and galactic BH candidates, like the typical asymmetric profile of the iron K line. Our assumptions (Kerr metric, disc illumination from a central source) may also yield a simple explanation of the K line equivalent width measured in some sources. In order to allow comparison with the data, we developed a computational tool aimed to fit the observed spectral features - including the disc-reflected continuum - on the base of fully relativistic models. The research we present here was performed under the supervision of V. Karas (AV R, Prague), E. Massaro (Uni1, Rome), G. Matt (Uni3, Rome), J. Miller (SISSA, Trieste). The present results were submitted as a Dissertation for the degree of Doctor Philosophiae at SISSA (Trieste), in October 2000. Bücher, Hörbücher & Kalender / Bücher / Sachbuch / Naturwissenschaften / Physik

2010, ISBN: 9783838391137

Erscheinungsdatum: 08/2010, Medium: Taschenbuch, Einband: Kartoniert / Broschiert, Titel: X-Ray Spectral Signatures of Accreting Black Holes, Titelzusatz: From the calculation of geodesics in the vicinity of spinning BHs to data analysis of real sources such as AGN and galactic BH candidates, Autor: Martocchia, Andrea, Verlag: LAP Lambert Acad. Publ., Sprache: Englisch, Rubrik: Physik // Astronomie, Sonstiges, Seiten: 164, Informationen: Paperback, Gewicht: 261 gr, Verkäufer: averdo Belletristik

2010, ISBN: 3838391136

Kartoniert / Broschiert, mit Schutzumschlag neu, [PU:LAP Lambert Acad. Publ.]