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20152026
most citedMAGNUM survey: Compact jets causing large turmoil in galaxies -- Enhanced line widths perpendicular to radio jets as tracers of jet-ISM interaction

142 citations · 758 across the 43 of their papers we have counts for

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Showing 2020Show all

9 papers · 1 filter

astro-ph.GA2020142 cited

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…

astro-ph.GA2020

The impact of the halo spin-concentration relation on disc scaling laws

Lorenzo Posti, Benoit Famaey, Gabriele Pezzulli +3

Galaxy scaling laws, such as the Tully-Fisher, mass-size and Fall relations, can provide extremely useful clues on our understanding of galaxy formation in a cosmological context.…

astro-ph.GA2020

The volumetric star formation law for nearby galaxies -- Extension to dwarf galaxies and low-density regions

Cecilia Bacchini, Filippo Fraternali, Gabriele Pezzulli +1

In the last decades, much effort has been put into finding the star formation law which could unequivocally link the gas and the star formation rate (SFR) densities measured on sub…

astro-ph.GA2020

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…

astro-ph.GA202070 cited

Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies

Cecilia Bacchini, Filippo Fraternali, Giuliano Iorio +3

It is well known that gas in galaxy discs is highly turbulent, but there is much debate on which mechanism can energetically maintain this turbulence. Among the possible candidates…

astro-ph.GA202035 cited

Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated

A. Marasco, L. Posti, K. Oman +3

We investigate the disc-halo connection in massive (Mstar/Msun>5e10) disc galaxies from the cosmological hydrodynamical simulations EAGLE and IllustrisTNG, and compare it with that…