The origin of UV-optical variability in AGN and test of disc models: XMM-Newton and ground-based observations of NGC 4395 Article

McHardy, IM, Connolly, SD, Peterson, BM et al. (2016). The origin of UV-optical variability in AGN and test of disc models: XMM-Newton and ground-based observations of NGC 4395 . 337(4-5), 500-506. 10.1002/asna.201612337

Open Access International Collaboration

cited authors

  • McHardy, IM; Connolly, SD; Peterson, BM; Bieryla, A; Chand, H; Elvis, MS; Emmanoulopoulos, D; Falco, E; Gandhi, P; Kaspi, S; Latham, D; Lira, P; McCully, C; Netzer, H; Uemura, M

authors

publication date

  • May 1, 2016

keywords

  • ACCRETION DISCS
  • ACTIVE GALACTIC NUCLEI
  • Astronomy & Astrophysics
  • BLACK-HOLE MASS
  • EMISSION
  • LONG
  • MCG-6-30-15
  • MR 2251-178
  • NGC-4051
  • Physical Sciences
  • SEYFERT-1 GALAXIES
  • Science & Technology
  • X-RAY VARIABILITY
  • X-rays: galaxies
  • accretion, accretion disks
  • black hole physics
  • galaxies: active
  • galaxies: individual (NGC 4395, NGC 5548)
  • galaxies: nuclei

Digital Object Identifier (DOI)

publisher

  • WILEY-V C H VERLAG GMBH

start page

  • 500

end page

  • 506

volume

  • 337

issue

  • 4-5