X-ray variability of 104 active galactic nuclei - XMM-Newton power-spectrum density profiles
By Omaira González-Martín, S. Vaughan. 2012
175 citations recorded by the source corpus.
archiveprefix: arXiv primaryclass: astro-ph.HE keywords: accretion, accretion disks, Galaxy: nucleus, galaxies: active, X-rays: galaxies eid: A80 adsurl: http://adsabs.harvard.edu/abs/2012A%26A...544A..80G adsnote: Provided by the SAO/NASA Astrophysics Data System
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/1c20c4debd179d79152d0589be9635e9640f717a
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Citations in the corpus
- Properties of flat-spectrum radio-loud Narrow-Line Seyfert 1 Galaxies (2014, background): “There are some relationships linking tb with the mass of the central black hole, the bolometric luminosity, or the FWHM of the Hβ (McHardy et al. 2006, González-Martín & Vaughan 2012).”
- A Multimessenger Picture of the Flaring Blazar TXS 0506+056: Implications for High-energy Neutrino Emission and Cosmic-Ray Acceleration (2018, background): “…gamma-ray bursts and supernovae, they are highly variable on different timescales and across the EM spectrum (Kataoka et al. 2001; Abdo et al. 2010; González-Martín & Vaughan 2012; Sobolewska et al. 2014), and have long been one of the most promising possibilities for HE neutrino production…”
- Active galactic nuclei: what’s in a name? (2017, background): “Although the exact functional dependence on the accretion rate/bolometric luminosity is currently debated (e.g. González-Martín and Vaughan 2012; Ponti et al. 2012), it is widely accepted that stellar-mass BHs in X-ray binary systems (BHXRBs) lie on the extension of the νb −MBH relation, which…”