Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-14T08:21:48.305Z Has data issue: false hasContentIssue false
  • English
  • Français

Rapid Line Variations in High Luminosity AGN and Anisotropic Emission of the Optical/UV Continuum

Published online by Cambridge University Press:  07 August 2017

M V Penston ,
E Pérez  and
M Moles
M V Penston
Affiliation:
Royal Greenwich Observatory, HAILSHAM, E Sussex, BN27 1RP, UK
E Pérez
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
M Moles
Affiliation:
Instituto de Astrofísica de Andalucia, Granada, Spain

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The emission lines of OVV quasars can vary significantly within a month, more rapidly than expected from photoionization models. This can be explained by anistropic continuum emission and joins several other lines of evidence suggesting anisotropic emission of the optical /uv continuum in AGN.

Type
Part 2: BLR and Variability
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 85 - 87
Copyright
Copyright © Kluwer 1989 

References

Antonucci, & Miller, , 1985. Ap.J., 297, 621.Google Scholar
Bregman, et al., 1986. Ap.J., 301, 698.Google Scholar
Browne, & Murphy, , 1986. M.N., 226, 601.Google Scholar
Gondhalekar, et al., 1987. RAL Workshop on AGN.Google Scholar
Malkan, & Sargent, , 1982. Ap.J., 254, 22.Google Scholar
Netzer, , 1987. M.N., 225, 55.Google Scholar
Orr, & Browne, , 1982. M.N., 200, 1067.Google Scholar
Pérez, et al., 1988a. M.N., 230, 353.Google Scholar
Pérez, et al., 1988b. This work.Google Scholar
Stephens, & Miller, , 1984. Bull. Ann. astr. Soc., 16, 1007.Google Scholar
Terrell, , 1966. Ap.J., 147, 827.Google Scholar
Unger, et al., 1987. M.N., 228, 671.Google Scholar
Wills, & Browne, , 1986. Ap.J., 302, 56.Google Scholar
Zheng, et al., 1987. Ap.J., 322, 164.Google Scholar