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Physics of ULIRGs with MUSE and ALMA: The PUMA project I. Properties of the survey and first MUSE data results
M. Perna, S. Arribas, M. Pereira Santaella +8
Ultraluminous infrared galaxies (ULIRGs) are characterised by extreme starburst (SB) and AGN activity, and are therefore ideal laboratories for studying the outflow phenomena. We h…
MAGNUM survey: Compact jets causing large turmoil in galaxies -- Enhanced line widths perpendicular to radio jets as tracers of jet-ISM interaction
G. Venturi, G. Cresci, A. Marconi +10
Outflows accelerated by AGN are commonly observed in the form of coherent, mildly collimated high-velocity gas directed along the AGN ionisation cones and kinetically powerful (>$1…
Galaxy-scale ionised winds driven by ultra-fast outflows in two nearby quasars
A. Marasco, G. Cresci, E. Nardini +14
We use MUSE adaptive optics (AO) data in Narrow Field Mode to study the properties of the ionised gas in MR 2251-178 and PG 1126-041, two nearby (z~0.06) bright quasars hosting sub…
MUSE view of Arp220: Kpc-scale multi-phase outflow and evidence for positive feedback
M. Perna, S. Arribas, C. Catalan-Torrecilla +9
Arp220 is the nearest and prototypical ULIRG, and shows evidence of pc-scale molecular outflows in its nuclear regions and strongly perturbed ionised gas kinematics on kpc scales.…
The peculiar emission line spectra of core-Extremely Red BOSS Quasars at 2-3: orientation and/or evolution?
Montse Villar Martin, Michele Perna, Andrew Humphrey +5
Core-extremely red quasars (core-ERQ) have been proposed to represent an intermediate evolutionary phase in which a heavily obscured quasar is blowing out the circumnuclear interst…