High- and Low-Velocity Magnetized Outflows in the Star Formation Process in a Gravitationally Collapsing Cloud

By Masahiro N. Machida, S. Inutsuka, Tomoaki Matsumoto. 2008

203 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Fluid Flow and Transfer Processes

View Paper: https://www.semanticscholar.org/paper/345bba165c145d7442da7149fb1734e6ed40944b

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Citations in the corpus

RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF PROTOSTELLAR COLLAPSE: PROTOSTELLAR CORE FORMATION (2012, methodology): “These are consistent with previous studies using the barotropic approximation (Machida et al. 2006a, 2007, 2008a).”
Magnetic Fields of Nondegenerate Stars (2009, background): “Simulations further suggest that clouds with higher magnetic fi lds may form first cores (and presumably protostars as well) containing less angular momentum (e.g., Hennebelle & Fromang 2008) and are less prone to fragmentation (e.g., Machida et al. 2008b; Hennebelle & Teyssier 2008).”
Effect of Magnetic Braking on Circumstellar Disk Formation in a Strongly Magnetized Cloud (2010, background): “This type of outflow was seen in many previous studies (e.g., Tomisaka 2002; Machida et al. 2004, 2005b; Machida et al. 2006, 2008b; Hennebelle & Fromang 2008; Duffin & Pudritz 2009; Tomida et al. 2010).”
Protostellar disk formation and transport of angular momentum during magnetized core collapse (2012, methodology): “The early formation of outflows during the collapse of dense cores was investigated recently by 2D and 3D MHD simulations (Mellon & Li 2008; Hennebelle & Fromang 2008), and where the second collapse was included (e.g. Banerjee et al. 2006; Machida et al. 2008).”
RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF PROTOSTELLAR COLLAPSE: NONIDEAL MAGNETOHYDRODYNAMIC EFFECTS AND EARLY FORMATION OF CIRCUMSTELLAR DISKS (2015, background): “…energy equations including the effects of radiation transfer, although radiation does not drastically affect the evolution in the early phase of star formation compared to the previous simulations using the barotropic approximation (e.g., Bate 1998; Saigo et al. 2008; Machida et al. 2008a, 2008b).”
Small-scale dynamo action during the formation of the first stars and galaxies - I. The ideal MHD limit (2010, methodology): “The impact of a uniformly imposed magnetic field (B0) in the primordial collapse has been studied by Machida et al. (2006, 2008) using direct numerical MHD simulations.”
Magnetic Fields in the Large-Scale Structure of the Universe (2011, background): “For simplified field geometries, Machida et al. (2006, 2008) found that magnetic fields lead to the formation of jets and help to suppress fragmentation in protostellar disks.”