SIMBAD references

2002MNRAS.337..861B - Mon. Not. R. Astron. Soc., 337, 861-868 (2002/December-2)

SPIRAL observations of the radio galaxy MRC B1733-565.

BRYANT J.J. and HUNSTEAD R.W.

Abstract (from CDS):

We present optical integral field spectroscopy of the elliptical host galaxy of MRC B1733-565 taken with SPIRAL on the Anglo-Australian Telescope. Emission-line gas is measured to be rotating about and extended perpendicular to the radio axis. To the south-east, the line emission reaches well beyond the continuum light from the galaxy, ending in a region of enhanced starburst activity, high density and disrupted gas flow. We suggest that this is an interacting gas and dust-rich starburst galaxy from which the AGN host is accreting gas along the extended emission-line region.

Abstract Copyright: RAS

Journal keyword(s): galaxies: active - galaxies: elliptical and lenticular, cD - galaxies: individual: MRC B1733-565 - galaxies: kinematics and dynamics - galaxies: Seyfert - galaxies: structure

Simbad objects: 1

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