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

188 citations · 1.5k across the 43 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.EP2022

Modelling photo-evaporation in planet forming discs

Barbara Ercolano, Giovanni Picogna

Planets are born from the gas and dust discs surrounding young stars. Energetic radiation from the central star can drive thermal outflows from the discs atmospheres, strongly affe…

astro-ph.EP20226 cited

The interplay between forming planets and photo-evaporating discs I: Forbidden line diagnostics

Michael L. Weber, Barbara Ercolano, Giovanni Picogna +1

Disc winds and planet formation are considered to be two of the most important mechanisms that drive the evolution and dispersal of protoplanetary discs and in turn define the envi…

astro-ph.IM202216 cited

Twinkle -- a small satellite spectroscopy mission for the next phase of exoplanet science

Ian Stotesbury, Billy Edwards, Jean-Francois Lavigne +35

With a focus on off-the-shelf components, Twinkle is the first in a series of cost competitive small satellites managed and financed by Blue Skies Space Ltd. The satellite is based…

astro-ph.EP202220 cited

The importance of X-ray frequency in driving photoevaporative winds

Andrew D. Sellek, Cathie J. Clarke, Barbara Ercolano

Photoevaporative winds are a promising mechanism for dispersing protoplanetary discs, but so far theoretical models have been unable to agree on the relative roles that the X-ray,…

astro-ph.EP202256 cited

Hydro-, Magnetohydro-, and Dust-Gas Dynamics of Protoplanetary Disks

G. Lesur, B. Ercolano, M. Flock +16

The building of planetary systems is controlled by the gas and dust dynamics of protoplanetary disks. While the gas is simultaneously accreted onto the central star and dissipated…

astro-ph.EP202212 cited

Observations of PAHs in the atmospheres of discs and exoplanets

Barbara Ercolano, Christian Rab, Karan Molaverdikhani +5

Polycyclic aromatic hydrocarbons (PAHs) play a key role in the chemical and hydrodynamical evolution of the atmospheres of exoplanets and planet-forming discs. If they can survive…