Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology - Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference, Held in Garching, Germany, 6-10 August 2001

The book reviews the present status of understanding the nature of the most luminous objects in the Universe, connected with supermassive black holes and supermassive stars, clusters of galaxies and ultraluminous galaxies, sources of gamma-ray bursts and relativistic jets. Leading experts give overviews of essential physical mechanisms involved, discuss formation and evolution of these objects as well as prospects for their use in cosmology, as probes of the intergalactic medium at high redshifts and as a tool to study the end of dark ages. The theoretical models are complemented by new exciting results from orbital and ground-based observatories such as Chandra, XMM-Newton, HST, SDSS, VLT, Keck, and many others.

Sommario

From the Contents: Clusters of Galaxies.- Brightest Galaxies.- Gamma-ray Bursts as the Lighthouses.- Gravitational Lensing and Gravitational Waves.- QSO, AGN, Blazars - Observational Data.- First Bright Objects and Their Role in the End of Dark Ages.- Formation and Growth of Supermassive BH.- Activity Connected with the Presence of Supermassive Black Holes.- Ultra-luminous X-ray Sources and Stellar Mass Black Holes.- QSO, AGN, Blazars as Probes of the Universe.- Lighthouses and the Cosmic Background Radiation.

Riassunto

The book reviews the present status of understanding the nature of the most luminous objects in the Universe, connected with supermassive black holes and supermassive stars, clusters of galaxies and ultraluminous galaxies, sources of gamma-ray bursts and relativistic jets. Leading experts give overviews of essential physical mechanisms involved, discuss formation and evolution of these objects as well as prospects for their use in cosmology, as probes of the intergalactic medium at high redshifts and as a tool to study the end of dark ages. The theoretical models are complemented by new exciting results from orbital and ground-based observatories such as Chandra, XMM-Newton, HST, SDSS, VLT, Keck, and many others.

Dettagli sul prodotto

• Con la collaborazione di: E. Churazov (Editore), Eugene Churazov (Editore), M. Gilfanov (Editore), Marat Gilfanov (Editore), R. Sunyaev (Editore), Rashid Sunyaev (Editore)
• Editore: Springer, Berlin
• Lingue: Inglese
• Formato: Copertina rigida
• Pubblicazione: 26.06.2009
• EAN: 9783540437697
• ISBN: 978-3-540-43769-7
• Pagine: 618
• Peso: 1221 g
• Illustrazioni: XIV, 618 p.
• Serie: ESO Astrophysics Symposia; ESO Astrophysics Symposia
• Categorie: Scienze naturali, medicina, informatica, tecnica > Fisica, astronomia > Astronomia; Gravitation, C, Galaxy, astronomy, Gravity, universe, Redshift, Astronomy, Astrophysics and Cosmology, Cosmology, Physics and Astronomy, Astronomy, Cosmology and Space Sciences, Observatory, black hole, stellar, Relativistic jet, active galactic nuclei, gamma-ray burst, Gravitational Waves, Galaxies, gravitational lens