most citedThe ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas

32 citations · 47 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Revealing the nature of the starburst galaxies in the overdensity HATLAS J0849

Melanie Kaasinen, Francesca Rizzo, Francesco Valentino +4

Today's most massive ellipticals are proposed to originate from starbursting galaxies in overdensities. To discern what triggers these starbursts, and their desce…

astro-ph.GA2026

Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes

Fernanda Roman-Oliveira, Francesca Rizzo, Filippo Fraternali

The rotation curves of regularly rotating disc galaxies are a unique probe of the gravitational potential and dark matter distribution. Until recently, matter decomposition of rota…

astro-ph.GA2026

Early thin-disc assembly revealed by JWST edge-on galaxies

Marloes van Asselt, Francesca Rizzo, Luca Di Mascolo

The vertical structure of stellar discs provides key constraints on their formation and evolution. Nearby spirals, including the Milky Way, host thin and thick components that may…

astro-ph.GA2024★ 32 cited

The ALMA-ALPAKA survey II. Evolution of turbulence in galaxy disks across cosmic time: difference between cold and warm gas

F. Rizzo, C. Bacchini, M. Kohandel +8

The gas in the interstellar medium (ISM) of galaxies is supersonically turbulent. Measurements of turbulence typically rely on cold gas emission lines for low-z galaxies and warm i…

astro-ph.GA2024

A 3D view on the local gravitational instability of cold gas discs in star-forming galaxies at

C. Bacchini, C. Nipoti, G. Iorio +6

Local gravitational instability (LGI) is considered crucial for regulating star formation and gas turbulence in galaxy discs, especially at high redshift. Instability criteria usua…

astro-ph.GA2024★ 15 cited

Dynamical modelling and origin of gas turbulence in z 4.5 galaxies

Fernanda Roman-Oliveira, Francesca Rizzo, Filippo Fraternali

In recent years, a growing number of regularly rotating galaxy discs have been found at z 4. Such systems provide us with the unique opportunity to study the properties of d…