Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology. Questo articolo non è disponibile.
Lingua: inglese
Editore: Springer, 2002
- Rilegato
- Nuovo

Da: Ria Christie Collections, Uxbridge, Regno UnitoRia Christie Collections
Venditore con 5 stelle
Venditore AbeBooks dal 25 marzo 2015
Non disponibile
Rilegato
Condizione: Nuovo
EUR 69,14
Descrizione dell’articolo da parte del venditore
In English.
Codice articolo ria9783540437697_new
- Titolo
- Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology
- Editore
- Springer
- Anno di pubblicazione
- 2002
- Condizione
- New
- Rilegatura
- Rilegato
- Lingua
- inglese
- ISBN 10
- 354043769X
- ISBN 13
- 9783540437697
- Peso dell'articolo
- 1182 grammi
- Serie
- Libro 4 di 12: ESO Astrophysics Symposia
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.
"Riassunto" può appartenere a un’altra edizione di questo titolo.
Dalla quarta di copertina
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.
"Descrizione articolo" può appartenere a un’altra edizione di questo titolo.