What controls the [O III] 5007 line strength in active galactic nuclei?
- 11 April 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 358 (3) , 1043-1054
- https://doi.org/10.1111/j.1365-2966.2005.08841.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 31 references indexed in Scilit:
- What controls the C iv line profile in active galactic nuclei?Monthly Notices of the Royal Astronomical Society, 2005
- Dusty, Radiation Pressure–Dominated Photoionization. II. Multiwavelength Emission Line Diagnostics for Narrow‐Line RegionsThe Astrophysical Journal Supplement Series, 2004
- Dusty, Radiation Pressure–Dominated Photoionization. I. Model Description, Structure, and GridsThe Astrophysical Journal Supplement Series, 2004
- Size and Structure of the Narrow-Line Region of QuasarsThe Astrophysical Journal, 2002
- Are the Narrow‐Line Regions in Active Galaxies Dusty and Radiation Pressure Dominated?The Astrophysical Journal, 2002
- Locally Optimally Emitting Clouds and the Narrow Emission Lines in Seyfert GalaxiesThe Astrophysical Journal, 1997
- The emission-line properties of low-redshift quasi-stellar objectsThe Astrophysical Journal Supplement Series, 1992
- VLA observations of objects in the Palomar Bright Quasar SurveyThe Astronomical Journal, 1989
- IUE spectra and a resulting model of Seyfert 2 galaxiesThe Astrophysical Journal, 1986
- Emission-line profiles and kinematics of the narrow-line region in Seyfert and radio galaxiesThe Astrophysical Journal, 1981