Astron. Astrophys. 334, 427-438 (1998)
The group of galaxies around 3C 275.1
J. Krempe -Krygier 1,
B. Krygier 2 and
G. Walentynowicz 2
1 N. Copernicus Astronomical Center, Astrophysical Lab.,
Toru , Poland
2 Toru Centre for
Astronomy, Toru , Poland
Received 23 April 1997 / Accepted 28 January 1998
Abstract
We have found that the quasar 3C275.1 is located at the centre of
the gravitational well of a group of galaxies characterized by
relativistic radial velocity and velocity dispersion equal to 124414
and 297 respectively.
The temperature of the ICM gas calculated from the "
" model is about K.
We suggest that there is a cooling flow in the ICM at a deposition
rate of about . It supplies gas to the
narrow-emission line region, in which the number density is equal to
0.4 and for homogeneous region and clouds of
radii of 10 respectively. The 1.6 GHz
European VLBI Network image of the quasar core shows the elongation of
radio structure at a distance from the core with
a position angle about . It may be the result of
interactions between out-flowing plasma of the QSO and the nonuniform
ionized gas emitting in forbidden [OII] and [OIII] emission lines. The
non-collinearity of the radio structure of 3C 275.1 might be explained
by an oblique shock of the plasma jet at the interface with the halo
of a neighbouring galaxy or with clouds of ionized gas.
Key words: galaxies: clusters: individual: A
98
quasars: individual: 3C
275.1
cooling flows
galaxies: jets
intergalactic
medium
radio continuum: galaxies
Send offprint requests to: J. Krempe -Krygier
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© European Southern Observatory (ESO) 1998
Online publication: May 15, 1998
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