[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 …
Molecules with ALMA at Planet-forming Scales (MAPS). I. Program overview and highlights
Planets form and obtain their compositions in dust-and gas-rich disks around young stars,
and the outcome of this process is intimately linked to the disk chemical properties. The …
and the outcome of this process is intimately linked to the disk chemical properties. The …
A highly settled disk around oph163131
M Villenave, KR Stapelfeldt, G Duchêne… - The Astrophysical …, 2022 - iopscience.iop.org
High dust density in the midplane of protoplanetary disks is favorable for efficient grain
growth and can allow fast formation of planetesimals and planets, before disks dissipate …
growth and can allow fast formation of planetesimals and planets, before disks dissipate …
Molecules with ALMA at Planet-forming Scales (MAPS). IV. Emission surfaces and vertical distribution of molecules
The Molecules with ALMA at Planet-forming Scales (MAPS) Large Program provides a
unique opportunity to study the vertical distribution of gas, chemistry, and temperature in the …
unique opportunity to study the vertical distribution of gas, chemistry, and temperature in the …
Molecules with ALMA at Planet-forming Scales (MAPS). II. CLEAN strategies for synthesizing images of molecular line emission in protoplanetary disks
The Molecules with ALMA at Planet-forming Scales Large Program (MAPS LP) surveyed the
chemical structures of five protoplanetary disks across more than 40 different spectral lines …
chemical structures of five protoplanetary disks across more than 40 different spectral lines …
Molecules with ALMA at planet-forming scales (MAPS). III. Characteristics of radial chemical substructures
The Molecules with ALMA at Planet-forming Scales (MAPS) Large Program provides a
detailed, high-resolution (∼ 10–20 au) view of molecular line emission in five protoplanetary …
detailed, high-resolution (∼ 10–20 au) view of molecular line emission in five protoplanetary …
Early Planet Formation in Embedded Disks (eDisk). II. Limited Dust Settling and Prominent Snow Surfaces in the Edge-on Class I Disk IRAS 04302+ 2247
While dust disks around optically visible, Class II protostars are found to be vertically thin,
when and how dust settles to the midplane are unclear. As part of the Atacama Large …
when and how dust settles to the midplane are unclear. As part of the Atacama Large …
Molecules with ALMA at Planet-forming Scales (MAPS). XVIII. Kinematic Substructures in the Disks of HD 163296 and MWC 480
We explore the dynamical structure of the protoplanetary disks surrounding HD 163296 and
MWC 480 as part of the Molecules with ALMA at Planet-forming Scales (MAPS) large …
MWC 480 as part of the Molecules with ALMA at Planet-forming Scales (MAPS) large …
Dust growth and evolution in protoplanetary disks
T Birnstiel - Annual Review of Astronomy and Astrophysics, 2023 - annualreviews.org
Over the past decade, advancement of observational capabilities, specifically the Atacama
Large Millimeter/submillimeter Array (ALMA) and Spectro-Polarimetric High-contrast …
Large Millimeter/submillimeter Array (ALMA) and Spectro-Polarimetric High-contrast …
DustPy: a python package for dust evolution in protoplanetary disks
SM Stammler, T Birnstiel - The Astrophysical Journal, 2022 - iopscience.iop.org
Many processes during the evolution of protoplanetary disks and during planet formation are
highly sensitive to the sizes of dust particles that are present in the disk: the efficiency of dust …
highly sensitive to the sizes of dust particles that are present in the disk: the efficiency of dust …