Formation and evolution of disks around young stellar objects

B Zhao, K Tomida, P Hennebelle, JJ Tobin… - Space Science …, 2020 - Springer
Recent observations have suggested that circumstellar disks may commonly form around
young stellar objects. Although the formation of circumstellar disks can be a natural result of …

Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy

EF van Dishoeck, LE Kristensen, JC Mottram… - Astronomy & …, 2021 - aanda.org
Context. Water is a key molecule in the physics and chemistry of star and planet formation,
but it is difficult to observe from Earth. The Herschel Space Observatory provided …

Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets

J Drazkowska, B Bitsch, M Lambrechts… - arXiv preprint arXiv …, 2022 - arxiv.org
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …

Early Planet Formation in Embedded Disks (eDisk). VII. Keplerian Disk, Disk Substructure, and Accretion Streamers in the Class 0 Protostar IRAS 16544–1604 in CB …

M Kido, S Takakuwa, K Saigo, N Ohashi… - The Astrophysical …, 2023 - iopscience.iop.org
We present observations of the Class 0 protostar IRAS 16544–1604 in CB 68 from the" Early
Planet Formation in Embedded Disks (eDisk)" ALMA Large program. The ALMA …

Questioning the spatial origin of complex organic molecules in young protostars with the CALYPSO survey

A Belloche, AJ Maury, S Maret, S Anderl… - Astronomy & …, 2020 - aanda.org
Context. Complex organic molecules (COMs) have been detected in a few Class 0
protostars but their origin is not well understood. While the usual picture of a hot corino …

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 …

Recent progress with observations and models to characterize the magnetic fields from star-forming cores to protostellar disks

A Maury, P Hennebelle, JM Girart - Frontiers in Astronomy and Space …, 2022 - frontiersin.org
In this review article, we aim at providing a global outlook on the progresses made in the
recent years to characterize the role of magnetic fields during the embedded phases of the …

The CALYPSO IRAM-PdBI survey of jets from Class 0 protostars-Exploring whether jets are ubiquitous in young stars

L Podio, B Tabone, C Codella, F Gueth… - Astronomy & …, 2021 - aanda.org
Aims. As a part of the CALYPSO Large Program, we aim to constrain the properties of
protostellar jets and outflows by searching for corresponding emission in a sample of 21 …

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Molecular Jets and Episodic Accretion in Protostars

S Dutta, CF Lee, D Johnstone, JE Lee… - The Astronomical …, 2024 - iopscience.iop.org
Protostellar outflows and jets are almost ubiquitous characteristics during the mass accretion
phase and encode the history of stellar accretion, complex organic molecule (COM) …

IPA: Class 0 Protostars Viewed in CO Emission Using JWST

AE Rubinstein, NJ Evans, H Tyagi… - The Astrophysical …, 2024 - iopscience.iop.org
We investigate the bright CO fundamental emission in the central regions of five protostars in
their primary mass assembly phase using new observations from JWST's Near-Infrared …