Jets are ubiquitous in the Universe and are seen from a large number of astrophysical objects including active galactic nuclei, gamma ray bursters, micro-quasars, proto-planetary …
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 …
Abstract We introduce the Disk Substructures at High Angular Resolution Project (DSHARP), one of the initial Large Programs conducted with the Atacama Large Millimeter/submillimeter …
Context. Previous theoretical works on planet formation around low-mass stars have often been limited to large planets and individual systems. As current surveys routinely detect …
M Ansdell, JP Williams, L Trapman… - The Astrophysical …, 2018 - iopscience.iop.org
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 …
We present the first part of our Disks ARound T Tauri Stars with SPHERE (DARTTS-S) survey: observations of eight T Tauri stars that were selected based on their strong (sub) …
J Huang, SM Andrews, CP Dullemond… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) used ALMA to map the 1.25 mm continuum of protoplanetary disks at a spatial resolution of∼ 5 au. We …
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 …
M Ansdell, JP Williams, CF Manara… - The Astronomical …, 2017 - iopscience.iop.org
The σ Orionis cluster is important for studying protoplanetary disk evolution, as its intermediate age (∼ 3–5 Myr) is comparable to the median disk lifetime. We use ALMA to …