activity
20162019
most citedChemical enrichment of giant planets and discs due to pebble drift

242 citations · 564 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.EP201947 cited

On the millimetre continuum flux-radius correlation of proto-planetary discs

Giovanni P. Rosotti, Richard A. Booth, Marco Tazzari +3

A correlation between proto-planetary disc radii and sub-mm fluxes has been recently reported. In this Letter we show that the correlation is a sensitive probe of grain growth proc…

astro-ph.EP2019101 cited

The time evolution of dusty protoplanetary disc radii: observed and physical radii differ

Giovanni P. Rosotti, Marco Tazzari, Richard A. Booth +3

Proto-planetary disc surveys conducted with ALMA are measuring disc radii in multiple star forming regions. The disc radius is a fundamental quantity to diagnose whether discs unde…

astro-ph.EP201844 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…

astro-ph.IM201752 cited

GANDALF - Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids

David A. Hubber, Giovanni P. Rosotti, Richard A. Booth

GANDALF is a new hydrodynamics and N-body dynamics code designed for investigating planet formation, star formation and star cluster problems. GANDALF is written in C++, parallelis…

astro-ph.SR201711 cited

Radiation-pressure-driven sub-Keplerian rotation of the disc around the AGB star L2 Pup

Thomas J. Haworth, Richard A. Booth, Ward Homan +3

We study the sub-Keplerian rotation and dust content of the circumstellar material around the asymptotic giant branch (AGB) star L Puppis. We find that the thermal pressure gra…

astro-ph.SR201710 cited

Chemical enrichment of the planet forming region as probed by accretion

Richard A. Booth, Cathie J. Clarke

The chemical conditions in the planet forming regions of protoplanetary discs remain difficult to observe directly. Gas accreting from the disc on to the star provides a way to mea…