This book presents timely work on the nature of the physical processes underpinning two of the basic characteristics of the gas structure in the innermost region of Active Galactic Nuclei (AGN): ionized outflows and emission line regions. In addition, it describes physics-based methods for estimating the density of the astrophysical plasma surrounding AGN. All numerical computations of the photoionized gas employ the most advanced codes available (CLOUDY and TITAN). Calculations of the radiative transfer are based on the assumption of thermal and ionization equilibrium.
Die Inhaltsangabe kann sich auf eine andere Ausgabe dieses Titels beziehen.
Dr Tek P Adhikari completed his MSc (Theoretical Physics) at Tribhuvan University in Kathmandu, Nepal in 2011. In 2018, he completed his PhD degree in Astronomy at the Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences (NCAC PAS) in Warsaw, Poland. Dr Adhikari’s doctoral dissertation was recognized with Distinction by the Scientific Council of the NCAC PAS for its outstanding contribution to the study of the AGN environment. In 2016, he received a Young Scientist Award from NCAC PAS for the best research paper by a Ph.D. student. He has delivered scientific talks at many international conferences and has co-authored more than 15 research publications in prestigious international journals.
„Über diesen Titel“ kann sich auf eine andere Ausgabe dieses Titels beziehen.
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
Zustand: New. In English. Artikel-Nr. ria9783030227364_new
Anzahl: Mehr als 20 verfügbar
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
Hardcover. Zustand: Brand New. 148 pages. 9.25x6.10x0.55 inches. In Stock. Artikel-Nr. x-3030227367
Anzahl: 2 verfügbar
Anbieter: Kennys Bookstore, Olney, MD, USA
Zustand: New. Artikel-Nr. V9783030227364
Anzahl: 15 verfügbar