FAUST–VIII. The protostellar disc of VLA 1623–2417W and its streamers imaged by ALMA
More than 50 per cent of solar-mass stars form in multiple systems. It is therefore crucial to
investigate how multiplicity affects the star and planet formation processes at the protostellar …
investigate how multiplicity affects the star and planet formation processes at the protostellar …
A millimeter-multiwavelength continuum study of VLA 1623 West
A Michel, SI Sadavoy, PD Sheehan… - The Astrophysical …, 2022 - iopscience.iop.org
VLA 1623 West is an ambiguous source that has been described as a shocked cloudlet as
well as a protostellar disk. We use deep ALMA 1.3 and 0.87 mm observations to constrain its …
well as a protostellar disk. We use deep ALMA 1.3 and 0.87 mm observations to constrain its …
FAUST XII. Accretion streamers and jets in the VLA 1623–2417 protocluster
The ALMA interferometer has played a key role in revealing a new component of the Sun-
like star forming process: the molecular streamers, ie structures up to thousands of au long …
like star forming process: the molecular streamers, ie structures up to thousands of au long …
Physical conditions for dust grain alignment in Class 0 protostellar cores-I. Observations of dust polarization and molecular irradiation tracers
Context. High angular resolution observations of Class 0 protostars have produced detailed
maps of the polarized dust emission in the envelopes of these young embedded objects …
maps of the polarized dust emission in the envelopes of these young embedded objects …
FAUST VI. VLA1623− 2417 B: a new laboratory for astrochemistry around protostars on 50 au scale
ABSTRACT The ALMA (Atacama Large Millimeter Array) interferometer, with its
unprecedented combination of high sensitivity and high angular resolution, allows for (sub-) …
unprecedented combination of high sensitivity and high angular resolution, allows for (sub-) …
Chemical and physical characterization of the isolated protostellar source CB68: FAUST IV
The chemical diversity of low-mass protostellar sources has so far been recognized, and
environmental effects are invoked as its origin. In this context, observations of isolated …
environmental effects are invoked as its origin. In this context, observations of isolated …
Fragmentation of dense rotation-dominated structures fed by collapsing gravo-magneto-sheetlets and origin of misaligned 100 au-scale binaries and multiple systems
The majority of stars are in binary/multiple systems. How such systems form in turbulent,
magnetized cores of molecular clouds in the presence of non-ideal magnetohydrodynamic …
magnetized cores of molecular clouds in the presence of non-ideal magnetohydrodynamic …
FAUST. VII. Detection of a Hot Corino in the Prototypical Warm Carbon-chain Chemistry Source IRAS 15398–3359
Y Okoda, Y Oya, L Francis, D Johnstone… - The Astrophysical …, 2023 - iopscience.iop.org
We have observed the low-mass protostellar source IRAS 15398− 3359 at a resolution of 0
farcs 2–0 farcs 3, as part of the Atacama Large Millimeter/Submillimeter Array Large …
farcs 2–0 farcs 3, as part of the Atacama Large Millimeter/Submillimeter Array Large …
Multiple misaligned outflows and warped accretion flows in the proto-multiple system Per-emb-8 and 55
SJ Lin, HW Yen, SP Lai - The Astronomical Journal, 2024 - iopscience.iop.org
To investigate the formation process of multiple systems, we have analyzed the Atacama
Large Millimeter/submillimeter Array archival data of the 1.3 mm continuum, 12 CO (2-1) and …
Large Millimeter/submillimeter Array archival data of the 1.3 mm continuum, 12 CO (2-1) and …
ATOMS: ALMA three-millimeter observations of massive star-forming regions–XIX. The origin of SiO emission
R Liu, T Liu, I Jiménez-Serra, JZ Li… - Monthly Notices of …, 2025 - academic.oup.com
The production of silicon monoxide (SiO) can be considered as a fingerprint of shock
interaction. In this work, we use high-sensitivity observations of the SiO (2–1) and H CO (1 …
interaction. In this work, we use high-sensitivity observations of the SiO (2–1) and H CO (1 …