activity
20062023
most citedPhotoevaporation of protoplanetary discs II: evolutionary models and observable properties

478 citations · 3.5k across the 54 of their papers we have counts for

collaborators

55 papers

astro-ph.SR2023★ 22 cited

The distribution of accretion rates as a diagnostic of protoplanetary disc evolution

R. Alexander, G. Rosotti, P. J. Armitage +3

We show that the distribution of observed accretion rates is a powerful diagnostic of protoplanetary disc physics. Accretion due to turbulent ("viscous") transport of angular momen…

astro-ph.SR2023★ 22 cited

The surprising evolution of the shadow on the TW Hya disk

J. Debes, R. Nealon, R. Alexander +8

We report new total intensity visible light high contrast imaging of the TW Hya disk taken with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST).…

astro-ph.SR2023★ 10 cited

Lyman-alpha Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems

Nicole Arulanantham, Max Gronke, Eleonora Fiorellino +18

T Tauri stars produce broad Lyman-alpha emission lines that contribute 88% of the total UV flux incident on the inner circumstellar disks. Lyman-alpha photons are generated a…

astro-ph.EP2022

Dust dynamics in planet-forming discs in binary systems

Francesco Zagaria, Giovanni P. Rosotti, Richard D. Alexander +1

In multiple stellar systems interactions among the companion stars and their discs affect planet formation. In the circumstellar case tidal truncation makes protoplanetary discs sm…

astro-ph.SR2022★ 5 cited

An unusual reservoir of water emission in the VV CrA A protoplanetary disk

Colette Salyk, Klaus M. Pontoppidan, Andrea Banzatti +7

We present an analysis of an unusual pattern of water vapor emission from the 2 Myr-old low-mass binary system VV CrA, as observed in infrared spectra obtained with VLT-CRIRE…

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…