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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

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18 papers · 1 filter

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.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.SR2022★ 37 cited

The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109

C. C. Espaillat, G. J. Herczeg, T. Thanathibodee +59

The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data fro…

astro-ph.SR2021★ 39 cited

Evidence for an MHD disk wind via optical forbidden line spectro-astrometry

E. T Whelan, I. Pascucci, U. Gorti +4

Spectro-astrometry is used to investigate the low velocity component (LVC) of the optical forbidden emission from the T Tauri stars RU Lupi and AS 205 N. Both stars also have high…