188 citations · 1.6k across the 51 of their papers we have counts for
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Large gaps and high accretion rates in photoevaporative transition disks with a dead zone
Matías Gárate, Timmy N. Delage, Jochen Stadler +7
Observations of young stars hosting transition disks show that several of them have high accretion rates, despite their disks presenting extended cavities in their dust component.…
The dispersal of protoplanetary discs. II: Photoevaporation models with observationally derived irradiating spectra
Barbara Ercolano, Giovanni Picogna, Kristina Monsch +2
Young solar-type stars are known to be strong X-ray emitters and their X-ray spectra have been widely studied. X-rays from the central star may play a crucial role in the thermodyn…
Presence of water on exomoons orbiting free-floating planets: a case study
Patricio Javier Ávila, Tommaso Grassi, Stefano Bovino +4
A free-floating planet is a planetary-mass object that orbits around a non-stellar massive object (e.g. a brown dwarf) or around the Galactic Center. The presence of exomoons orbit…
The imprint of X-ray photoevaporation of planet-forming discs on the orbital distribution of giant planets -- II. Theoretical predictions
Kristina Monsch, Giovanni Picogna, Barbara Ercolano +1
Numerical models have shown that disc dispersal via internal photoevaporation driven by the host star can successfully reproduce the observed pile-up of warm Jupiters near 1-2 au.…
Testing photoevaporation and MHD disk wind models through future high-angular resolution radio observations: the case of TW Hydrae
Luca Ricci, Sarah Harter, Barbara Ercolano +1
We present theoretical predictions for the free-free emission at cm wavelengths obtained from photoevaporation and MHD wind disk models adjusted to the case of the TW Hydrae young…
PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis
C. F. Manara, A. Frasca, L. Venuti +69
The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…