214 citations · 2.1k across the 38 of their papers we have counts for
8 papers · 1 filter
Can chondrules be produced by the interaction of Jupiter with the protosolar disk?
Jean-David Bodénan, Clément Surville, Judit Szulágyi +2
Chondrules are crystallised droplets of silicates formed by rapid heating to high temperatures (> 1800 K) of solid precursors followed by hours or days of cooling. Dating of chondr…
Formation of satellites in circumplanetary discs generated by disc instability
C. Inderbitzi, J. Szulágyi, M. Cilibrasi +1
We investigated the formation and evolution of satellite systems in a cold, extended circumplanetary disc around a 10 gas giant which was formed by gravitational…
RefPlanets: Search for reflected light from extra-solar planets with SPHERE/ZIMPOL
S. Hunziker, H. M. Schmid, D. Mouillet +55
RefPlanets is a guaranteed time observation (GTO) programme that uses the Zurich IMaging POLarimeter (ZIMPOL) of SPHERE/VLT for a blind search for exoplanets in wavelengths from 60…
Detection of H emission from PZ Tel B using SPHERE/ZIMPOL
Arianna Musso Barcucci, Gabriele Cugno, Ralf Launhardt +7
H is a powerful tracer of accretion and chromospheric activity, which has been detected in the case of young brown dwarfs and even recently in planetary mass companions (e.g. PD…
Dust production in the debris disk around HR 4796 A
J. Olofsson, J. Milli, P. Thébault +21
Debris disks are the natural by-products of the planet formation process. Scattered or polarized light observations are mostly sensitive to small dust grains that are released from…
ALMA observations require slower Core Accretion runaway growth
S. Nayakshin, G. Dipierro, J. Szulagyi
Thanks to recent high resolution ALMA observations, there is an accumulating evidence for presence of giant planets with masses from Jupiter mass to a few Jupiter mass…
Observability of Forming Planets and their Circumplanetary Disks II. -- SEDs and Near-Infrared Fluxes
J. Szulágyi, C. P. Dullemond, A. Pohl +1
Detection of forming planets means detection of the circumplanetary disk (CPD) in reality, since the planet is still surrounded by a disk at this evolutionary stage. Yet, no compre…
Masses and Distances of Planetary Microlens Systems with High Angular Resolution Imaging
Aparna Bhattacharya, Rachel Akeson, Jay Anderson +33
Microlensing is the only method that can detect and measure mass of wide orbit, low mass, solar system analog exoplanets. Mass measurements of such planets would yield massive scie…