128 citations · 526 across the 12 of their papers we have counts for
12 papers
LEGO II: A 3 mm molecular line study covering 100 pc of one of the most actively star-forming portions within the Milky Way Disc
A. T. Barnes, J. Kauffmann, F. Bigiel +20
The current generation of (sub)mm-telescopes has allowed molecular line emission to become a major tool for studying the physical, kinematic, and chemical properties of extragalact…
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…
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…
ALMA Observations of the Young Substellar Binary System 2M1207
L. Ricci, P. Cazzoletti, I. Czekala +10
We present ALMA observations of the 2M1207 system, a young binary made of a brown dwarf with a planetary-mass companion at a projected separation of about 40 au. We detect emission…
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…