activity
20122026
most citedEvidence for a correlation between mass accretion rates onto young stars and the mass of their protoplanetary disks

206 citations · 5.5k across the 195 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.EP2018★ 52 cited

Is the ring inside or outside the planet?: The effect of planet migration on dust rings

Farzana Meru, Giovanni P. Rosotti, Richard A. Booth +2

Planet migration in protoplanetary discs plays an important role in the longer term evolution of planetary systems, yet we currently have no direct observational test to determine…

astro-ph.EP2018★ 101 cited

High resolution millimetre imaging of the CI Tau protoplanetary disc - a massive ensemble of protoplanets from 0.1 - 100 au

Cathie J. Clarke, Marco Tazzari, Attila Juhász +8

We present high resolution millimeter continuum imaging of the disc surrounding the young star CI Tau, a system hosting the first hot Jupiter candidate in a protoplanetary disc sys…

astro-ph.SR2018★ 26 cited

Gaia DR2 view of the Lupus V-VI clouds: the candidate diskless young stellar objects are mainly background contaminants

C. F. Manara, T. Prusti, F. Comeron +10

Extensive surveys of star-forming regions with Spitzer have revealed populations of disk-bearing young stellar objects. These have provided crucial constraints, such as the timesca…

astro-ph.EP2018★ 30 cited

The comparative effect of FUV, EUV and X-ray disc photoevaporation on gas giant separations

Jeff Jennings, Barbara Ercolano, Giovanni P. Rosotti

Gas giants' early ( Myr) orbital evolution occurs in a disc losing mass in part to photoevaporation driven by high energy irradiance from the host star. This process ma…

astro-ph.SR2018★ 179 cited

Protoplanetary disc truncation mechanisms in stellar clusters: comparing external photoevaporation and tidal encounters

Andrew J. Winter, Cathie J. Clarke, Giovanni Rosotti +3

Most stars form and spend their early life in regions of enhanced stellar density. Therefore the evolution of protoplanetary discs (PPDs) hosted by such stars are subject to the in…

astro-ph.EP2018★ 44 cited

Protoplanetary Disc Response to Distant Tidal Encounters in Stellar Clusters

A. J. Winter, C. J. Clarke, G. Rosotti +1

The majority of stars form in a clustered environment. This has an impact on the evolution of surrounding protoplanetary discs (PPDs) due to either photoevaporation or tidal trunca…