144 citations · 1.9k across the 67 of their papers we have counts for
10 papers · 1 filter
GASP XXXII. Measuring the diffuse ionized gas fraction in ram-pressure stripped galaxies
Neven Tomicic, Benedetta Vulcani, Bianca M. Poggianti +8
The diffuse ionized gas (DIG) is an important component of the interstellar medium and it can be affected by many physical processes in galaxies. Measuring its distribution and con…
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…
The WISSH QSOs project IX. Cold gas content and environment of luminous QSOs at z~2.4-4.7
M. Bischetti, C. Feruglio, E. Piconcelli +23
Sources at the brightest end of QSO luminosity function during the peak epoch of star formation and black hole accretion (z~2-4, i.e. Cosmic noon) are privileged sites to study the…
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…
GASP XXX. The spatially resolved SFR-Mass relation in stripping galaxies in the local universe
B. Vulcani, B. M. Poggianti, S. Tonnesen +10
The study of the spatially resolved Star Formation Rate-Mass (Sigma_SFR-Sigma_M) relation gives important insights on how galaxies assemble at different spatial scales. Here we pre…
The high molecular gas content, and the efficient conversion of neutral into molecular gas, in jellyfish galaxies
A. Moretti, R. Paladino, B. M. Poggianti +11
In the disks of four jellyfish galaxies from the GASP sample at redshift we detect molecular gas masses systematically higher than in field galaxies. These galaxies are…