High-mass star and massive cluster formation in the milky way

F Motte, S Bontemps, F Louvet - Annual Review of Astronomy …, 2018 - annualreviews.org
This review examines the state-of-the-art knowledge of high-mass star and massive cluster
formation, gained from ambitious observational surveys, which acknowledges the multiscale …

The big problems in star formation: the star formation rate, stellar clustering, and the initial mass function

MR Krumholz - Physics Reports, 2014 - Elsevier
Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

Massive star formation

JC Tan, MT Beltrán, P Caselli, F Fontani… - … and Planets VI, 2014 - books.google.com
The enormous radiative and mechanical luminosities of massive stars impact a vast range of
scales and processes, from the reionization of the universe, to the evolution of galaxies, to …

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

P Sanhueza, Y Contreras, B Wu… - The Astrophysical …, 2019 - iopscience.iop.org
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey:
Clump Fragmentation - IOPscience This site uses cookies. By continuing to use this site you …

The role of magnetic fields in setting the star formation rate and the initial mass function

MR Krumholz, C Federrath - Frontiers in Astronomy and Space …, 2019 - frontiersin.org
Star-forming gas clouds are strongly magnetized, and their ionization fractions are high
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …

Magnetic fields in star formation: from clouds to cores

K Pattle, L Fissel, M Tahani, T Liu… - arxiv preprint arxiv …, 2022 - arxiv.org
In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …

Physical processes in star formation

P Girichidis, SSR Offner, AG Kritsuk, RS Klessen… - Space Science …, 2020 - Springer
Star formation is a complex multi-scale phenomenon that is of significant importance for
astrophysics in general. Stars and star formation are key pillars in observational astronomy …

Comparing the pre-SNe feedback and environmental pressures for 6000 H ii regions across 19 nearby spiral galaxies

AT Barnes, SCO Glover, K Kreckel… - Monthly Notices of …, 2021 - academic.oup.com
The feedback from young stars (ie pre-supernova) is thought to play a crucial role in
molecular cloud destruction. In this paper, we assess the feedback mechanisms acting …

Magnetic fields in high-mass infrared dark clouds

T Pillai, J Kauffmann, JC Tan… - The Astrophysical …, 2015 - iopscience.iop.org
High-mass stars are cosmic engines known to dominate the energetics in the Milky Way and
other galaxies. However, their formation is still not well understood. Massive, cold, dense …

Collapse of turbulent massive cores with ambipolar diffusion and hybrid radiative transfer-I. Accretion and multiplicity

R Mignon-Risse, M González, B Commerçon… - Astronomy & …, 2021 - aanda.org
Context. Massive stars form in magnetized and turbulent environments and are often located
in stellar clusters. The accretion and outflows mechanisms associated with forming massive …