activity
20122025
most citedAccretion of Jupiter-mass Planets in the Limit of Vanishing Viscosity

214 citations · 2.1k across the 38 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.SR2018★ 16 cited

Mapping of shadows cast on a protoplanetary disk by a close binary system

V. D'Orazi, R. Gratton, S. Desidera +47

For a comprehensive understanding of planetary formation and evolution, we need to investigate the environment in which planets form: circumstellar disks. Here we present high-cont…

astro-ph.SR2018★ 80 cited

High-Resolution ALMA Observations of HD100546: Asymmetric Circumstellar Ring, and Circumplanetary Disk Upper Limits

J. E. Pineda, J. Szulágyi, S. P. Quanz +7

We present long baseline Atacama Large Millimeter/submillimeter Array (ALMA) observations of the 870m dust continuum emission and CO (3-2) from the protoplanetary disk around…

astro-ph.EP2018★ 37 cited

In Situ Formation of Icy Moons of Uranus and Neptune

J. Szulágyi, M. Cilibrasi, L. Mayer

Satellites of giant planets thought to form in gaseous circumplanetary disks (CPDs) during the late planet-formation phase, but it was unknown so far whether smaller mass planets,…

astro-ph.SR2018★ 121 cited

Evolution of protoplanetary disks from their taxonomy in scattered light: spirals, rings, cavities, and shadows

Antonio Garufi, Myriam Benisty, Paola Pinilla +11

The variety of observed protoplanetary disks in polarimetric light motivates a taxonomical study to constrain their evolution and establish the current framework of this type of ob…

astro-ph.EP2018★ 35 cited

Dust evolution and satellitesimal formation in circumplanetary disks

Joanna Drazkowska, Judit Szulágyi

It is believed that satellites of giant planets form in circumplanetary disks. Many of the previous contributions assumed that their formation process proceeds similarly to rocky p…

astro-ph.EP2018★ 34 cited

New disk discovered with VLT/SPHERE around the M star GSC 07396-00759

E. Sissa, J. Olofsson, A. Vigan +30

Debris disks are usually detected through the infrared excess over the photospheric level of their host star. The most favorable stars for disk detection are those with spectral ty…

astro-ph.EP2018★ 31 cited

Satellites Form Fast & Late: a Population Synthesis for the Galilean Moons

M. Cilibrasi, J. Szulágyi, L. Mayer +3

The satellites of Jupiter are thought to form in a circumplanetary disc. Here we address their formation and orbital evolution with a population synthesis approach, by varying the…