A&A 371, 507-511 (2001)
DOI: 10.1051/0004-6361:20010404
A two-phase model for the narrow line region of NGC 4151
S. KomossaMax-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany
(Received 9 February 2001 / Accepted 16 March 2001)
Abstract
NGC 4151 is one of the brightest and best-studied
Seyfert galaxies. Here, we present a two-phase model of
the narrow-line region (NLR) of NGC 4151.
This study is motivated by (i) the fact that the
X-ray spectrum of NGC 4151 is among the flattest known
for Seyferts, and (ii) the recent Chandra
detection of an X-ray narrow-line
region in this galaxy.
X-ray spectra as flat as that of NGC 4151 (
)
are expected to favor the presence
of two gas phases in pressure equilibrium (Krolik et al. 1981).
In the present study, we show that a
pronounced two-phase equilibrium develops in the extended emission-line region
if we use
the observed multi-wavelength spectrum of NGC 4151
to ionize the clouds.
The material is stable to isobaric perturbations over
a wide range of temperatures.
We therefore propose that such a condition
has arisen in the NLR of NGC 4151, and that it explains
the detection of hot,
extended X-ray gas which we identify as the NLR-cloud
confining medium.
Key words: galaxies: Seyfert -- galaxies: individual: NGC 4151 -- galaxies: nuclei -- galaxies: emission lines -- X-rays: galaxies
Offprint request: S. Komossa, skomossa@xray.mpe.mpg.de
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