activity
20172026
most citedProtoplanetary disc `isochrones' and the evolution of discs in the plane

96 citations · 145 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2026

Azimuthal brightness modulation reveals hidden rings in CI Tau

C. E. Scardoni, G. P. Rosotti, F. Zagaria +4

Protoplanetary disks often host substructures such as rings and gaps, which trace key processes in planet formation and dust evolution. However, narrow rings may remain unresolved…

astro-ph.EP2025

Eccentric discs as a gateway to giant planets outward migration

Chiara E. Scardoni, Giovanni P. Rosotti, Cathie J. Clarke +2

Recent studies on planet-dominated Type II migration demonstrated the presence of a correlation between the direction of planet migration and the parameter K describing the depth o…

astro-ph.EP2024★ 7 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.EP2022★ 14 cited

Inward and outward migration of massive planets: moving towards a stalling radius

C. E. Scardoni, C. J. Clarke, G. P. Rosotti +3

Recent studies on the planet-dominated regime of Type II migration showed that, contrary to the conventional wisdom, massive planets can migrate outwards. Using `fixed-planet' simu…

astro-ph.EP2021★ 12 cited

The effect of the streaming instability on protoplanetary disc emission at millimetre wavelengths

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

In this paper, we investigate whether overdensity formation via streaming instability is consistent with recent multi-wavelength ALMA observations in the Lupus star forming region.…

astro-ph.SR2020★ 1 cited

X-Shooter survey of disk accretion in Upper Scorpius I. Very high accretion rates at age>5 Myr

C. F. Manara, A. Natta, G. P. Rosotti +14

Determining the mechanisms that drive the evolution of protoplanetary disks is a necessary step to understand how planets form. Here we measured the mass accretion rate for young s…