The signature of high velocity gas in the spectra of NGC 4151
arXiv:astro-ph/0202146 · doi:10.1051/0004-6361:20020245
Abstract
The multiwavelength emission spectrum and associated velocity field of the Seyfert prototype NGC 4151 is modeled. HST data has impressively revealed the existence of a large range of velocities (100 - 1500 \kms) dominating the emitting clouds in the extended emission line region of the galaxy. Following this observational result, a revision of the photoionization modeling approach applied to NGC 4151 is presented. It is concluded that a mixture of radiation dominated clouds and shock dominated clouds are required to explain the multiwavelength line and continuum spectra of the galaxy.
arXiv comment16 pages, LaTeX class for Astronomy and Astrophysics (including 3 Tables) + 8 PostScript figures. To appear in "Astronomy and Astrophysics"
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- The 3-5 micron Spectrum of NGC 1068 at High Angular Resolution: Distribution of Emission and Absorption Features across the Nuclear Continuum Source
- The Narrow Line Region of Ark 564
- Spectra from the shocked nebulae revealing turbulence near the Galactic Centre
- The LLAGN in the centre of the Galaxy
- The Infrared-X-ray continuum correlation in Active Galactic Nuclei