-
Articles citing this article
-
Same authors
- Recommend this article
- Download citation
- Alert me if this article is cited
- Alert me if this article is corrected
|
||||||||||||||||||
A&A 439, 935-946 (2005)
DOI: 10.1051/0004-6361:20041609
The HST view of the nuclear emission line region in low luminosity radio-galaxies
A. Capetti1, G. V. Kleijn2 and M. Chiaberge31 INAF - Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy
e-mail: capetti@to.astro.it
2 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany
e-mail: gverdoes@eso.org
3 INAF - Istituto di Radioastronomia, via Gobetti 101, 40129 Bologna, Italy
e-mail: chiab@ira.cnr.it
(Received 7 July 2004 / Accepted 5 April 2005)
Abstract
We study the properties of the emission line regions in two
samples of low luminosity radio-galaxies, while focusing on the
Compact Emission Line Region (CELR) revealed to be a characteristic
feature of these objects by HST narrow-band imaging.
We find a strong correlation between line and optical
continuum nuclear emission, which suggests that the optical cores (most
likely of non-thermal origin) can be directly associated to the source
of ionizing photons, i.e. that we are seeing a jet-ionized narrow line
region. A photon budget argument indicates that the optical nuclear
sources produce sufficient photon flux provided that the covering
factor of the circum-nuclear gas is rather large, on average ~0.3.
Analysis of HST images and spectra suggests that
the CELR may take the form of a pc-scale, high filling factor
structure, possibly an optically thin torus.
Estimates of the CELR mass lead to values as small as
, and photon counting sets a limit to the Broad Line Region
mass of
. When considered together with the low accretion
rate and the tenuous torus structure, a general paucity of gas in the
innermost regions of low luminosity radio-galaxies
emerges as the main characterizing
difference from more powerful Active Galactic Nuclei.
Key words: galaxies: active -- galaxies: nucleus -- galaxies: jets
SIMBAD Objects
© ESO 2005
| What is OpenURL? |
- If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
- You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
- You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.

BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook