No evidence for large-scale outflows in the extended ionised halo of ULIRG Mrk273
arXiv:1603.00488 · doi:10.1093/mnrasl/slw033
Abstract
We present deep new GTC/OSIRIS narrow-band images and optical WHT/ISIS long-slit spectroscopy of the merging system Mrk273 that show a spectacular extended halo of warm ionised gas out to a radius of kpc from the system nucleus. Outside of the immediate nuclear regions (r > 6 kpc), there is no evidence for kinematic disturbance in the ionised gas: in the extended regions covered by our spectroscopic slits the emission lines are relatively narrow (FWHM 350 km) and velocity shifts small (|V| 250 km). This is despite the presence of powerful near-nuclear outflows (FWHM > 1000 km; |V| > 400 km; r < 6 kpc). Diagnostic ratio plots are fully consistent with Seyfert 2 photo-ionisation to the NE of the nuclear region, however to the SW the plots are more consistent with low-velocity radiative shock models. The kinematics of the ionised gas, combined with the fact that the main structures are aligned with low-surface-brightness tidal continuum features, are consistent with the idea that the ionised halo represents tidal debris left over from a possible triple-merger event, rather than a reservoir of outflowing gas.
arXiv comment5 pages, 3 figures, accepted for publication in MNRAS Letters
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- The small observed scale of AGN--driven outflows, and inside--out disc quenching
- Massive outflow properties suggest AGN fade slowly
- Chemical abundances of Seyfert 2 AGNs IV. Composite models calculated by photoionization + shocks
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- KCWI observations of the extended nebulae in Mrk 273
- Seeing the forest and the trees: a radio investigation of the ULIRG Mrk 273