activity
20192026
most citedThe evolution of dust in discs influenced by external photoevaporation

90 citations · 444 across the 28 of their papers we have counts for

collaborators
Showing 2025Show all

11 papers · 1 filter

astro-ph.EP2025★ 5 cited

Photoevaporation Can Reproduce Extended Emission from Protoplanetary Disks Imaged by JWST MIRI

R. Nakatani, G. Rosotti, B. Tabone +1

Understanding dispersal of protoplanetary disks remains a central challenge in planet formation theory. Disk winds, driven by magnetohydrodynamics (MHD) and/or photoevaporation, ar…

astro-ph.EP2025★ 9 cited

Understanding JWST water spectra: what can thermochemical models tell us about the (cold) water in protoplanetary disks?

Marissa Vlasblom, Milou Temmink, Andrew D. Sellek +1

(Abridged) Rotational HO spectra as observed with JWST/MIRI provide a good probe of the temperature and column density structure of the inner disk. HO emission can also be…

astro-ph.EP2025★ 17 cited

A transition from HO to CH dominated spectra with decreasing stellar luminosity

Sierra L. Grant, Milou Temmink, Ewine F. van Dishoeck +19

The chemical composition of the inner regions of disks around young stars will determine the properties of planets forming there. Many disk physical processes drive the chemical ev…

astro-ph.EP2025★ 5 cited

MINDS. Young binary systems with JWST/MIRI: Variable water-rich primaries and extended emission

Nicolas T. Kurtovic, Sierra L. Grant, Milou Temmink +16

As part of the JWST GTO program MINDS, we analyze the mid-infrared emission of three Class II binary systems: VW Cha, WX Cha, and RW Aur, to investigate the impact of stellar multi…

astro-ph.EP2025★ 11 cited

Chemical transformation of CO in evolving protoplanetary discs across stellar masses: a route to C-rich inner regions

Andrew D. Sellek, Ewine F. van Dishoeck

Protoplanetary discs around Very Low Mass Stars (VLMS) show hydrocarbon-rich MIR spectra indicative of C/O>1 in their inner discs, in contrast to discs around higher-mass hosts whi…

astro-ph.EP2025★ 1 cited

A correlation between accretion and outflow rates for Class II Young Stellar Objects with full and transition disks

A. A. Rota, N. van der Marel, A. Garufi +7

Magnetothermal (MHD) winds and jets originate in a wide range of regions of protoplanetary disks (1-30 au) and are thought to be the primary mechanisms driving accretion onto the c…