The Physics and Evolution of Active Galactic Nuclei: The AGN family

By H. Netzer. 2013

277 citations recorded by the source corpus.

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Citations in the corpus

Black holes, gravitational waves and fundamental physics: a roadmap (2018, background): “longer [595], and are dominant in the case of SMBBH systems.”
The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe (2014, methodology): “We refer readers to the texts of Krolik (1999), Netzer (2013), Osterbrock & Ferland (2005), Peterson (1997), and the review by Yuan & Narayan in this volume, for the gory details.”
BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog (2017, background): “…keV have shown that the shape of the CXB is significantly flatter (with a photon index Γ ∼ 1.4, e.g., De Luca & Molendi 2004) than * cricci@astro.puc.cl 24 See Beckmann & Shrader (2012); Netzer (2013, 2015); Brandt & Alexander (2015); Ramos Almeida & Ricci (2017) for recent reviews on the subject.”
Physical Models of Galaxy Formation in a Cosmological Framework (2014, background): “These seed BH may grow by accreting gas that either has negligible angular momentum, or by forming an accretion disk that drains the gas of angular momentum via viscosity (Netzer 2013).”
Nuclear activity versus star formation: emission-line diagnostics at ultraviolet and optical wavelengths (2015, methodology): “In fact, some authors appeal to very high metallicities (up to Z ∼ 10Z ) to reproduce observations (Netzer 2013).”
EVIDENCE FOR WIDE-SPREAD ACTIVE GALACTIC NUCLEUS-DRIVEN OUTFLOWS IN THE MOST MASSIVE z ∼ 1–2 STAR-FORMING GALAXIES (2014, background): “A possible alternative, and formally also acceptable decomposition of the specific co-added nuclear spectrum in the left panel of Figure 4 is obtained if one assumes that the broad emission is due to Hα only, as would be expected for BLR emission (see Netzer 2013).”
x-cigale: fitting AGN/galaxy SEDs from X-ray to infrared (2020, unknown): “E-mail: gyang206265@gmail.com (GY) different physical processes (e.g. Netzer 2013).”
Cool outflows in galaxies and their implications (2020, background): “from the AGN (Barvainis 1987; Netzer 2013).”
Revisiting the Unified Model of Active Galactic Nuclei (2015, background): “Almost all type-I AGNs show Compton humps in their spectra (the terms “scattering” and “reflection” are used quite loosely in the literature, all referring to Compton scattering followed by absorption, see e.g. Netzer (1993)).”
SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. II. SWIFT AND HST REVERBERATION MAPPING OF THE ACCRETION DISK OF NGC 5548 (2015, unknown): “56) of Netzer (2013). However, these derivations all assume a relatively flat disk.”
SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. III. OPTICAL CONTINUUM EMISSION AND BROADBAND TIME DELAYS IN NGC 5548 (2015, background): “On the other hand, a comparison of ṁE can be made assuming a thin-disk spectrum and using the observed optical luminosity (e.g., Collin et al. 2002; Netzer 2013, Equation (4.53)).”
Fast radio bursts (2018, background): “For example, radio sources were identified with galaxies that have jets, double-lobed radio emitting regions and active nuclei (“quasars”) [45].”