| 书目名称 | Photoionization Modelling as a Density Diagnostic of Line Emitting/Absorbing Regions in Active Galactic Nuclei |
| 编辑 | Tek Prasad Adhikari |
| 视频video | |
| 概述 | Nominated as an outstanding PhD thesis by the Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw, Poland.Provides a general overview of the latest research on Active Gal |
| 丛书名称 | Springer Theses |
| 图书封面 |  |
| 描述 | 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. Promising preliminary examples of comparison with current observations are included for several individual AGN. All of them suggest that the absorbing/emitting gas should have a density on the order of 10.12. cm.-3.. Future observations will provide more objects to verify these results, and will allow us to put constraints on the launch radius of ionized outflows and therefore on the mass loading and kinetic energy outflow rates. These rates, in turn, are crucial to estimating whether the outflows have a significant feedback impact on star formation and metal enrichment in the interstellar medium of the host galaxy. |
| 出版日期 | Book 2019 |
| 关键词 | Photoionization Modelling; Warm Absorbers; TITAN code simulations; CLOUDY code simulations; Absorption M |
| 版次 | 1 |
| doi | https://doi.org/10.1007/978-3-030-22737-1 |
| isbn_softcover | 978-3-030-22739-5 |
| isbn_ebook | 978-3-030-22737-1Series ISSN 2190-5053 Series E-ISSN 2190-5061 |
| issn_series | 2190-5053 |
| copyright | Springer Nature Switzerland AG 2019 |
发表于 2025-3-21 17:53:14
