Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows II

Highly-ionized fast accretion-disk winds have been suggested as an explanation for a variety of observed absorption and emission features in the X-ray spectra of Active Galactic Nuclei. Simple estimates have suggested that these flows may be massive enough to carry away a significant fraction of the...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy: Sim, SA, Miller, L, Long, K, Turner, T, Reeves, J
Format: Journal article
Język:English
Wydane: 2010