activity
20162026
most citedThe prevalence of star formation as a function of Galactocentric radius

41 citations · 178 across the 18 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.GA2024★ 13 cited

Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust

J. D. Soler, S. Molinari, S. C. O. Glover +10

We present a reconstruction of the line-of-sight motions of the local interstellar medium (ISM) based on the combination of a model of the three-dimensional dust density distributi…

astro-ph.GA2024★ 30 cited

Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters

M. R. A. Wells, H. Beuther, S. Molinari +47

We use data from the ALMA Evolutionary Study of High Mass Protocluster Formation in the Galaxy (ALMAGAL) survey to study 100 ALMAGAL regions at 1 arsecond resolution located…

astro-ph.EP2024★ 4 cited

The evolution of the and correlations traces protoplanetary disc dispersal

Alice Somigliana, Leonardo Testi, Giovanni Rosotti +9

(Abridged) Observational surveys of entire star-forming regions have provided evidence of power-law correlations between the disc properties and the stellar mass, especially the di…

astro-ph.SR2024

The chemistry of star and planet formation with SKA

C. Codella, L. Testi, G. Umana +2

In this contribution, we aim to summarise the efforts of the Italian SKA scientific community in conducting surveys of star-forming regions within our Galaxy, in the development of…

astro-ph.EP2024★ 16 cited

Accuracy of ALMA estimates of young disk radii and masses. Predicted observations from numerical simulations

Ngo-Duy Tung, Leonardo Testi, Ugo Lebreuilly +7

Protoplanetary disks, which are the natural consequence of the gravitational collapse of the dense molecular cloud cores, host the formation of the known planetary systems in our u…