2010, ISBN: 3838391136

[EAN: 9783838391137], Neubuch, [PU: LAP LAMBERT Academic Publishing], nach der Bestellung gedruckt Neuware -The calculation of (general-relativistic) geodesics in the vicinity of spinning… Mehr…

[EAN: 9783838391137], Neubuch, [PU: LAP LAMBERT Academic Publishing], nach der Bestellung gedruckt 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, Books<

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 … Mehr…

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 geodesic… Mehr…

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: 9783838391137

Paperback, Neubuch, BRAND NEW BOOK! Shipped within 24-48 hours. Normal delivery time is 5-12 days. Please note some orders may be shipped from UK with same delivery timeframe, ***NO EXPED… Mehr…

Paperback, Neubuch, BRAND NEW BOOK! Shipped within 24-48 hours. Normal delivery time is 5-12 days. Please note some orders may be shipped from UK with same delivery timeframe, ***NO EXPEDITED ORDERS***, [PU: LAP LAMBERT Academic Publishing]<

2010, ISBN: 9783838391137

Trade paperback, New., Trade paperback (US). Glued binding. 164 p., [PU: LAP Lambert Academic Publishing]