Ambipolar diffusion in low-mass star formation - I. General comparison with the ideal magnetohydrodynamic case

By J. Masson, G. Chabrier, P. Hennebelle, N. Vaytet, B. Commerccon. 2015

136 citations recorded by the source corpus.

We thank the anonymous referee for the suggestions and remarks that contributed to improve the quality of this manuscript. The research leading to these results has received funding from the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007-2013 Grant Agreement no. 247060). B.C. gratefully acknowledges support from the French ANR Retour Postdoc program (ANR-11-PDOC-0031). We finally acknowledge financial support from the “Programme National de Physique Stellaire” (PNPS) of CNRS/INSU, France.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/84141a03b9b832151bc56288aae1f95baa1326fd

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Citations in the corpus

The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. II. A Statistical Characterization of Class 0 and Class I Protostellar Disks (2020, background): “…processes (i.e., ohmic dissipation, the Hall effect, and ambipolar diffusion) are now regularly included in numerical codes and enable the formation of disks during the protostellar phase (e.g., Dapp & Basu 2010; Li et al. 2011; Machida & Matsumoto 2011; Hennebelle et al. 2016; Masson et al. 2016).”