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20032026
most citedX-ray irradiated protoplanetary disk atmospheres I: Predicted emission line spectrum and photoevaporation

188 citations · 1.6k across the 51 of their papers we have counts for

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Showing 2021Show all

11 papers · 1 filter

astro-ph.EP202141 cited

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.…

astro-ph.EP202170 cited

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…

astro-ph.EP202123 cited

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…

astro-ph.EP2021

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.…

astro-ph.EP2021

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…

astro-ph.SR2021

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…