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

188 citations · 1.5k across the 45 of their papers we have counts for

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Showing 2020Show all

7 papers · 1 filter

astro-ph.EP202047 cited

A highly non-Keplerian protoplanetary disc: Spiral structure in the gas disc of CQ Tau

Lisa Wölfer, Stefano Facchini, Nicolas T. Kurtovic +9

In the past years, high angular resolution observations have revealed that circumstellar discs appear in a variety of shapes with diverse substructures being ubiquitous. This has g…

astro-ph.SR202056 cited

The interpretation of protoplanetary disc wind diagnostic lines from X-ray photoevaporation and analytical MHD models

Michael L. Weber, Barbara Ercolano, Giovanni Picogna +2

High resolution spectra of typical wind diagnostics ([OI] 6300 Å and other forbidden emission lines) can often be decomposed into multiple components: high-velocity components with…

astro-ph.EP20207 cited

Modelling thermochemical processes in protoplanetary disks I: numerical methods

T. Grassi, B. Ercolano, L. Szűcs +2

The dispersal phase of planet-forming disks via winds driven by irradiation from the central star and/or magnetic fields in the disk itself is likely to play an important role in t…

astro-ph.EP2020

Solid accretion onto planetary cores in radiative disks

Apostolos Zormpas, Giovanni Picogna, Barbara Ercolano +1

The solid accretion rate, necessary to grow gas giant planetary cores within the disk lifetime, has been a major constraint for theories of planet formation. We tested the solid ac…

physics.pop-ph2020

Extrasolar planets: from dust to new worlds

Barbara Ercolano

Thousands of exoplanets have been discovered and the search for life outside Earth is at the forefront of astrophysical research. The planets we observe show a mind-blowing diversi…

astro-ph.EP2020

Hydrogen recombination line luminosities and -variability from forming planets

J. Szulágyi, B. Ercolano

We calculated hydrogen recombination line luminosities (H-, Paschen- and Brackett-) from three dimensional thermo-hydrodynamical simulations of forming planets from 1 to 1…