PRODIGE–Planet-forming disks in Taurus with NOEMA-II. Modeling the CO (2–1) isotopologue emission of the Class II T Tauri disks in Taurus
R Franceschi, T Henning… - Astronomy & …, 2024 - aanda.org
Context. To understand how planets form in protoplanetary disks, it is necessary to
characterize their gas and dust distribution and masses. This requires a combination of high …
characterize their gas and dust distribution and masses. This requires a combination of high …
Dust Drift Timescales in Protoplanetary Disks at the Cusp of Gravitational Instability
JP Williams, C Painter, AR Anderson… - The Astrophysical …, 2024 - iopscience.iop.org
Millimeter emitting dust grains have sizes that make them susceptible to drift in
protoplanetary disks due to the difference between their orbital speed and that of the gas …
protoplanetary disks due to the difference between their orbital speed and that of the gas …
PRODIGE–envelope to disk with NOEMA-IV. An infalling gas bridge surrounding two Class 0/I systems in L1448N
Context. The formation of stars has been subject to extensive studies in the past decades on
scales from molecular clouds to proto-planetary disks. It is still not fully understood how the …
scales from molecular clouds to proto-planetary disks. It is still not fully understood how the …