Demographics of young stars and their protoplanetary disks: lessons learned on disk evolution and its connection to planet formation
Since Protostars and Planets VI (PPVI), our knowledge of the global properties of
protoplanetary and debris disks, as well as of young stars, has dramatically improved. At the …
protoplanetary and debris disks, as well as of young stars, has dramatically improved. At the …
[HTML][HTML] Empirical constraints on turbulence in proto-planetary discs
GP Rosotti - New Astronomy Reviews, 2023 - Elsevier
Proto-planetary discs, the birth environment of planets, are an example of a structure
commonly found in astrophysics, accretion discs. Identifying the mechanism responsible for …
commonly found in astrophysics, accretion discs. Identifying the mechanism responsible for …
ALMA survey of lupus protoplanetary disks. II. Gas disk radii
Abstract We present Atacama Large Millimeter/Sub-Millimeter Array (ALMA) Band 6
observations of a complete sample of protoplanetary disks in the young (∼ 1–3 Myr) Lupus …
observations of a complete sample of protoplanetary disks in the young (∼ 1–3 Myr) Lupus …
Secular evolution of MHD wind-driven discs: analytical solutions in the expanded α-framework
B Tabone, GP Rosotti, AJ Cridland… - Monthly Notices of …, 2022 - academic.oup.com
The evolution of protoplanetary discs and the related process of planet formation is
regulated by angular momentum transport and mass-loss processes. Over the past decade …
regulated by angular momentum transport and mass-loss processes. Over the past decade …
The external photoevaporation of planet-forming discs
Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
Lupus disks with faint CO isotopologues: low gas/dust or high carbon depletion?
Context. An era has started in which gas and dust can be observed independently in
protoplanetary disks, thanks to the recent surveys with the Atacama Large Millimeter/sub …
protoplanetary disks, thanks to the recent surveys with the Atacama Large Millimeter/sub …
MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus
The final architecture of planetary systems depends on the extraction of angular momentum
and mass-loss processes of the discs in which they form. Theoretical studies proposed that …
and mass-loss processes of the discs in which they form. Theoretical studies proposed that …
The protoplanetary disk population in the ρ-Ophiuchi region L1688 and the time evolution of Class II YSOs
L Testi, A Natta, CF Manara… - Astronomy & …, 2022 - aanda.org
Context. Planets form during the first few Myr of the evolution of the star-disk system,
possibly before the end of the embedded phase. The properties of very young disks and …
possibly before the end of the embedded phase. The properties of very young disks and …
The Mass Accretion Rate and Stellar Properties in Class I Protostars
E Fiorellino, Ł Tychoniec, FCS de Miera… - The Astrophysical …, 2023 - iopscience.iop.org
Stars collect most of their mass during the protostellar stage, yet the accretion luminosity and
stellar parameters, which are needed to compute the mass accretion rate, are poorly …
stellar parameters, which are needed to compute the mass accretion rate, are poorly …
On the secular evolution of the ratio between gas and dust radii in protoplanetary discs
ABSTRACT A key problem in protoplanetary disc evolution is understanding the efficiency of
dust radial drift. This process makes the observed dust disc sizes shrink on relatively short …
dust radial drift. This process makes the observed dust disc sizes shrink on relatively short …