128 citations · 526 across the 12 of their papers we have counts for
6 papers · 1 filter
Revealing the dust grain size in the inner envelope of the Class I protostar Per-emb-50
C. Agurto-Gangas, J. E. Pineda, L. Szucs +7
A good constraint of when the growth of dust grains from sub-micrometer to millimeter sizes occurs, is crucial for planet formation models. This provides the first step towards the…
An ALMA Survey of faint disks in the Chamaeleon I star-forming region: Why are some Class II disks so faint?
Feng Long, Gregory J. Herczeg, Ilaria Pascucci +6
ALMA surveys of nearby star-forming regions have shown that the dust mass in the disk is correlated with the stellar mass, but with a large scatter. This scatter could indicate eit…
Gravitational instabilities in a protosolar-like disc II: continuum emission and mass estimates
M. G. Evans, J. D. Ilee, T. W. Hartquist +6
Gravitational instabilities (GIs) are most likely a fundamental process during the early stages of protoplanetary disc formation. Recently, there have been detections of spiral fea…
Cold CO gas in the disk of the young eruptive star EX Lup
Ágnes Kóspál, Péter Ábrahám, Timea Csengeri +6
EX Lupi-type objects (EXors) form a sub-class of T Tauri stars, defined by sudden sporadic flare-ups of 1-5 magnitudes at optical wavelengths. These eruptions are attributed to enh…
The Herschel/PACS view of disks around low-mass stars in Chamaleon-I
J. Olofsson, L. Szűcs, Th. Henning +3
Circumstellar disks are expected to be the birthplaces of planets. The potential for forming one or more planets of various masses is essentially driven by the initial mass of the…
Stellar-Mass-Dependent Disk Structure in Coeval Planet-Forming Disks
László Szűcs, Dániel Apai, Ilaria Pascucci +1
Previous studies suggest that the planet-forming disks around very-low-mass stars/brown dwarfs may be flatter than those around more massive stars, in contrast to model predictions…