AGN outflows are integral for understanding how the central super massive black hole interacts with the host galaxy and co-evolves in cosmic time. This white paper sets the primary science goals for the next decade and suggests the key parameters on which the next generation X-ray telescopes should be built to revolutionize our understanding.
The physics and astrophysics of X-ray outflows from Active Galactic Nuclei / Laha, ., Sibasish, ., Smith, ., Randall, ., Tzanavaris, ., Panayiotis, ., Kallman, ., Tim, ., Veilleux, ., Sylvain, ., Tombesi, ., Francesco, ., Kriss, ., Gerard, ., Guainazzi, ., Matteo, ., Gaspari, M., Kaastra, ., Jelle, ., Markowitz, ., et al.. - In: BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY. - ISSN 2330-9458. - 51:3(2019).
The physics and astrophysics of X-ray outflows from Active Galactic Nuclei
GASPARI M;
2019
Abstract
AGN outflows are integral for understanding how the central super massive black hole interacts with the host galaxy and co-evolves in cosmic time. This white paper sets the primary science goals for the next decade and suggests the key parameters on which the next generation X-ray telescopes should be built to revolutionize our understanding.
| File | Dimensione | Formato | |
|---|---|---|---|
|
075_laha.pdf
Accesso riservato
Dimensione
192.47 kB
Formato
Adobe PDF
|
192.47 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
Pubblicazioni consigliate
I metadati presenti in IRIS UNIMORE sono rilasciati con licenza Creative Commons CC0 1.0 Universal, mentre i file delle pubblicazioni sono rilasciati con licenza Attribuzione 4.0 Internazionale (CC BY 4.0), salvo diversa indicazione.
In caso di violazione di copyright, contattare Supporto Iris
