SPIRAL observations of the radio galaxy MRC B1733-565

Details SPIRAL observations of the radio galaxy MRC B1733-565 SPIRAL observations of the radio galaxy MRC B1733-565

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.337..861b&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 337, Issue 3, pp. 861-868.

Astronomy and Astrophysics

Astronomy

3

Galaxies: Active, Galaxies: Elliptical And Lenticular, Cd, Galaxies: Individual: Mrc B1733-565, Galaxies: Kinematics And Dynamics, Galaxies: Seyfert, Galaxies: Structure

Scientific paper

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.

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