Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-06-24T08:08:00.502Z Has data issue: false hasContentIssue false

Intermediate Resolution Hβ Spectroscopy and Photometric Monitoring of 3C 390.3. I. Further Evidence of a Nuclear Accretion Disk

Published online by Cambridge University Press:  12 April 2016

L. Carrasco
Affiliation:
Instituto Nacional de Astrofisica, Optica y Electronica, Apartado Postal 51. C.P. 72000, Puebla, Pue., Mexico
V.H. Chavushyan
Affiliation:
Instituto Nacional de Astrofisica, Optica y Electronica, Apartado Postal 51. C.P. 72000, Puebla, Pue., Mexico
J.R. Valdes
Affiliation:
Instituto Nacional de Astrofisica, Optica y Electronica, Apartado Postal 51. C.P. 72000, Puebla, Pue., Mexico
F. Legrand
Affiliation:
Instituto Nacional de Astrofisica, Optica y Electronica, Apartado Postal 51. C.P. 72000, Puebla, Pue., Mexico
V.T. Doroshenko
Affiliation:
Sternberg Astronomical Institute, University of Moscow, Universitetskij Prospect 13, Moscow 119899, Russia
V.M. Lyuty
Affiliation:
Sternberg Astronomical Institute, University of Moscow, Universitetskij Prospect 13, Moscow 119899, Russia
N.G. Bochkarev
Affiliation:
Sternberg Astronomical Institute, University of Moscow, Universitetskij Prospect 13, Moscow 119899, Russia
A-M. Dumont
Affiliation:
DAEC, Observatorie de Paris, section de Meudon, Place Jansen, F-92195 Meudon, France
S. Collin
Affiliation:
DAEC, Observatorie de Paris, section de Meudon, Place Jansen, F-92195 Meudon, France
O. Kurtanidze
Affiliation:
Abastumani Observatory, Republic of Georgia
M.G. Nikolashvili
Affiliation:
Abastumani Observatory, Republic of Georgia

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 variations of the Hβ broad emission line and continuum flux in 3C 390.3 are investigated. Our results favor the formation of the broad Hβ line of 3C 390.3 n an accretion disk.

Type
Part 5. AGN Phenomena
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Eracleous, M., et al. 1997, ApJ, 490, 216 CrossRefGoogle Scholar
Shapovalova, A.I., et al. 2001, A&A, 376, 775 Google Scholar