activity
20142023
most citedPolytropic models of filamentary interstellar clouds - I. Structure and stability

38 citations · 85 across the 4 of their papers we have counts for

collaborators

11 papers

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.EP20244 cited

Angular momentum transport via gravitational instability in the Elias 2-27 disc

Cristiano Longarini, Giuseppe Lodato, Cathie J. Clarke +6

Gravitational instability is thought to be one of the main drivers of angular momentum transport in young protoplanetary discs. The disc around Elias 2-27 offers a unique example o…

astro-ph.SR2024

Full orbital solutions in pre-main sequence high-order multiple systems: GG Tau Ab and UX Tau B

Gaspard Duchêne, Jean-Baptiste LeBouquin, François Ménard +3

High-order multiple (triple and beyond) systems are relatively common. Their interaction with circumstellar and circumbinary material can have a large impact on the formation and e…

astro-ph.EP202316 cited

The time evolution of in protoplanetary discs as a way to disentangle between viscosity and MHD winds

Alice Somigliana, Leonardo Testi, Giovanni Rosotti +5

As the classic viscous paradigm for protoplanetary disk accretion is challenged by the observational evidence of low turbulence, the alternative scenario of MHD disk winds is being…

astro-ph.EP20235 cited

Radio multiwavelength analysis of the compact disk CX Tau: Presence of strong free-free variability or anomalous microwave emission

Pietro Curone, Leonardo Testi, Enrique Macias +8

Protoplanetary disks emit radiation across a broad range of wavelengths, requiring a multiwavelength approach to fully understand their physical mechanisms and how they form planet…