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Turbulence-induced disc formation in strongly...
Preprint

Turbulence-induced disc formation in strongly magnetised cloud cores

Abstract

We present collapse simulations of strongly magnetised, turbulent molecular cloud cores with masses ranging from 2.6 to 1000 M_sun in order to study the

Authors

Seifried D; Banerjee R; Pudritz RE; Klessen RS

Publication date

February 20, 2013

DOI

10.48550/arxiv.1302.4901

Preprint server

arXiv