activity
20142024
most citedOn the gas content of transitional disks: a VLT/X-Shooter study of accretion and winds

168 citations · 827 across the 29 of their papers we have counts for

collaborators

31 papers

astro-ph.EP20243 cited

The emergence of the Md-Macc correlation in the MHD wind scenario

Luigi Zallio, Giovanni Rosotti, Benoît Tabone +3

There is still much uncertainty around the mechanism that rules the accretion of proto-planetary disks. In the last years, Magnetohydrondynamic (MHD) wind-driven accretion has been…

astro-ph.SR20249 cited

A tell-tale tracer for externally irradiated protoplanetary disks: comparing the [CI] 8727 A line and ALMA observations in proplyds

Mari-Liis Aru, Karina Mauco, Carlo F. Manara +15

The evolution of protoplanetary disks in regions with massive OB stars is influenced by externally driven winds that deplete the outer parts of disks. These winds have previously b…

astro-ph.EP20244 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.EP20244 cited

Planet-driven spirals in protoplanetary discs: limitations of the semi-analytical theory for observations

D. Fasano, A. J. Winter, M. Benisty +7

Detecting protoplanets during their formation stage is an important but elusive goal of modern astronomy. Kinematic detections via the spiral wakes in the gaseous disc are a promis…

astro-ph.EP20247 cited

Seeing the unseen: a method to detect unresolved rings in protoplanetary disks

Chiara E. Scardoni, Richard A. Booth, Cathie J. Clarke +2

While high resolution ALMA observations reveal a wealth of substructure in protoplanetary discs, they remain incapable of resolving the types of small scale dust structures predict…

astro-ph.EP202414 cited

DBNets: A publicly available deep learning tool to measure the masses of young planets in dusty protoplanetary discs

Alessandro Ruzza, Giuseppe Lodato, Giovanni Pietro Rosotti

Current methods to characterize embedded planets in protoplanetary disc observations are severely limited either in their ability to fully account for the observed complex physics…