Collapse of Massive Magnetized Dense Cores Using Radiation Magnetohydrodynamics: Early Fragmentation Inhibition

We report the results of radiation-magnetohydrodynamics calculations in the context of high-mass star formation, using for the first time a self-consistent model for photon emission (i.e., via thermal emission and in radiative shocks) and with the high resolution necessary to properly resolve magnet...

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Bibliographic Details
Published in:Astrophysical journal. Letters 2011-11, Vol.742 (1), p.L9-jQuery1323914751411='48'
Main Authors: Commerçon, Benoît, Hennebelle, Patrick, Henning, Thomas
Format: Article
Language:English
Subjects:
ANGULAR MOMENTUM
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
CARBON MONOXIDE
FEEDBACK
GRAVITATIONAL COLLAPSE
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
MASS
PHOTON EMISSION
Physics
RADIANT HEAT TRANSFER
RESOLUTION
STAR CLUSTERS
STARS
TURBULENCE
VELOCITY
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Summary:We report the results of radiation-magnetohydrodynamics calculations in the context of high-mass star formation, using for the first time a self-consistent model for photon emission (i.e., via thermal emission and in radiative shocks) and with the high resolution necessary to properly resolve magnetic braking effects and radiative shocks on scales
ISSN:2041-8205
2041-8213
DOI:10.1088/2041-8205/742/1/L9