617 citations · 5.1k across the 84 of their papers we have counts for
8 papers · 1 filter
High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and CH emission
T. Paneque-Carreño, A. F. Izquierdo, R. Teague +4
Constraining turbulence in disks is key towards understanding their evolution through the transport of angular momentum. Until now measurements of high turbulence have remained elu…
A dusty streamer infalling onto the disk of a class I protostar. ALMA dual-band constraints on grain properties and mass infall rate
L. Cacciapuoti, E. Macias, A. Gupta +15
Observations of interstellar material infalling onto star- and planet-forming systems have become increasingly common thanks to recent advancements in radio interferometry. These s…
Millimeter emission in photoevaporating disks is determined by early substructures
Matías Gárate, Til Birnstiel, Paola Pinilla +7
[abridged]Photoevaporation and dust-trapping are individually considered to be important mechanisms in the evolution and morphology of protoplanetary disks. We studied how the pres…
The VLT MUSE NFM view of outflows and externally photoevaporating discs near the Orion Bar
Thomas J. Haworth, Megan Reiter, C. Robert O'Dell +10
We present VLT/MUSE Narrow Field Mode (NFM) observations of a pair of disc-bearing young stellar objects towards the Orion Bar: 203-504 and 203-506. Both of these discs are subject…
FAUST IX. Multi-band, multi-scale dust study of L1527 IRS. Evidence for dust properties variations within the envelope of a Class 0/I YSO
L. Cacciapuoti, E. Macias, A. J. Maury +25
Early dust grain growth in protostellar envelopes infalling on young discs has been suggested in recent studies, supporting the hypothesis that dust particles start to agglomerate…
Testing protoplanetary disc evolution with CO fluxes. A proof of concept in Lupus and Upper Sco
Francesco Zagaria, Stefano Facchini, Anna Miotello +3
The Atacama Large Millimeter/submillimeter Array (ALMA) revolutionised our understanding of protoplanetary discs. However, the available data have not given conclusive answers yet…