Issue |
A&A
Volume 446, Number 3, February II 2006
|
|
---|---|---|
Page(s) | 919 - 932 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20053571 | |
Published online | 20 January 2006 |
Size and properties of the NLR in the Seyfert-2 galaxy NGC 1386
1
Astronomisches Institut Ruhr-Universität Bochum, Universitätsstrasse 150, 44780 Bochum, Germany e-mail: [nbennert;haas;chini]@astro.rub.de
2
Astronomical Institute, Academy of Sciences of the Czech Republic, Boční II 1401, 141 31 Prague 4, Czech Republic e-mail: bruno@ig.cas.cz
3
CRAL-Observatoire de Lyon, 9 avenue Charles André, 69561 Saint-Genis-Laval Cedex, France
4
Max-Planck Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany e-mail: skomossa@xray.mpe.mpg.de
Received:
3
June
2005
Accepted:
3
October
2005
We study the narrow-line region (NLR)
of the Seyfert-2 galaxy NGC 1386
by means of long-slit spectroscopy obtained with FORS1 at the VLT.
We use the galaxy itself for subtracting the stellar template, applying
reddening corrections to fit the stellar template to the spectra of the
NLR. The continuum gets steadily redder towards the nucleus. The spatial
distribution of the reddening derived from the Balmer decrement differs from the
continuum reddening, indicating dust within the NLR with a
varying column density along the
line of sight. Using spatially resolved spectral diagnostics,
we find a transition between central line ratios falling into the
AGN regime and outer ones
in the -region regime, occuring at a radius of ~6´´ (310
pc) in all three diagnostic diagrams.
Applying CLOUDY photoionisation models, we show that the observed distinction
between
-like and AGN-like ratios in NGC 1386 represents a true
difference in ionisation source and cannot
be explained by variations of physical parameters such as
ionisation parameter, electron density or metallicity. We
interpret it as a real border between the NLR,
i.e. the central AGN-photoionised region and
surrounding
regions.
We derive surface brightness,
electron density, and ionisation parameter
as a function of distance from the
nucleus. Both the electron density and the ionisation parameter decrease with
radius. We discuss the consequences of these observations
for the interpretation of the empirical NLR size-luminosity relation.
In the outer part of the NLR, we find evidence for shocks, resulting in a
secondary peak of the electron-density and ionisation-parameter distribution
north of the nucleus. We compare the NLR velocity curve with the stellar one
and discuss the differences.
Key words: galaxies: active / galaxies: individual: NGC 1386 / galaxies: nuclei / galaxies: Seyfert
© ESO, 2006
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