From filamentary networks to dense cores in molecular clouds: toward a new paradigm for star formation
P André, J Di Francesco… - … and Planets VI, 2014 - books.google.com
Recent studies of the nearest star-forming clouds of the Galaxy at submillimeter wavelengths
with the Herschel Space Observatory have provided us with unprecedented images of the …
with the Herschel Space Observatory have provided us with unprecedented images of the …
The origin of the stellar mass distribution and multiplicity
YN Lee, SSR Offner, P Hennebelle, P André… - Space Science …, 2020 - Springer
In this chapter, we review some historical understanding and recent advances on the Initial
Mass Function (IMF) and the Core Mass Function (CMF), both in terms of observations and …
Mass Function (IMF) and the Core Mass Function (CMF), both in terms of observations and …
Radiation magnetohydrodynamic simulations of protostellar collapse: nonideal magnetohydrodynamic effects and early formation of circumstellar disks
The transport of angular momentum by magnetic fields is a crucial physical process in the
formation and evolution of stars and disks. Because the ionization degree in star-forming …
formation and evolution of stars and disks. Because the ionization degree in star-forming …
A HERSCHEL* AND APEX CENSUS OF THE REDDEST SOURCES IN ORION: SEARCHING FOR THE YOUNGEST PROTOSTARS
AM Stutz, JJ Tobin, T Stanke, ST Megeath… - The Astrophysical …, 2013 - iopscience.iop.org
We perform a census of the reddest, and potentially youngest, protostars in the Orion
molecular clouds using data obtained with the PACS instrument on board the Herschel …
molecular clouds using data obtained with the PACS instrument on board the Herschel …
Early planet formation in embedded disks (eDisk). IX. High-Resolution ALMA observations of the class 0 protostar R CrA IRS5N and its surroundings
R Sharma, JK Jørgensen, S Gavino… - The Astrophysical …, 2023 - iopscience.iop.org
We present high-resolution high-sensitivity observations of the Class 0 protostar RCrA
IRS5N as part of the Atacama Large Milimeter/submilimeter Array large program Early …
IRS5N as part of the Atacama Large Milimeter/submilimeter Array large program Early …
Collapse of a molecular cloud core to stellar densities: stellar-core and outflow formation in radiation magnetohydrodynamic simulations
We have performed smoothed particle radiation magnetohydrodynamic simulations of the
collapse of rotating, magnetized molecular cloud cores to form protostars. The calculations …
collapse of rotating, magnetized molecular cloud cores to form protostars. The calculations …
The Earliest Phases of Star Formation (EPoS): a Herschel key project-The thermal structure of low-mass molecular cloud cores
R Launhardt, AM Stutz, A Schmiedeke… - Astronomy & …, 2013 - aanda.org
Context. The temperature and density structure of molecular cloud cores are the most
important physical quantities that determine the course of the protostellar collapse and the …
important physical quantities that determine the course of the protostellar collapse and the …
The impact of non-ideal magnetohydrodynamic processes on discs, outflows, counter-rotation, and magnetic walls during the early stages of star formation
J Wurster, MR Bate, IA Bonnell - Monthly Notices of the Royal …, 2021 - academic.oup.com
Non-ideal magnetohydrodynamic (MHD) processes–namely Ohmic resistivity, ambipolar
diffusion, and the Hall effect–modify the early stages of the star formation process and the …
diffusion, and the Hall effect–modify the early stages of the star formation process and the …
Herschel observations of B1-bS and B1-bN: two first hydrostatic core candidates in the Perseus star-forming cloud
S Pezzuto, D Elia, E Schisano, F Strafella… - Astronomy & …, 2012 - aanda.org
We report far-infrared Herschel observations obtained between 70 μm and 500 μm of two
star-forming dusty condensations,[HKM99] B1-bS and [HKM99] B1-bN, in the B1 region of …
star-forming dusty condensations,[HKM99] B1-bS and [HKM99] B1-bN, in the B1 region of …
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Discovery of an extremely dense and compact object embedded in the prestellar core G208. 68 …
N Hirano, D Sahu, SY Liu, T Liu… - The Astrophysical …, 2024 - iopscience.iop.org
The internal structure of the prestellar core G208. 68-19.02-N2 (G208-N2) in the Orion
Molecular Cloud 3 (OMC-3) region has been studied with the Atacama Large Millimeter …
Molecular Cloud 3 (OMC-3) region has been studied with the Atacama Large Millimeter …