An analysis of the turbulence in the central region of M 42 through structure functions

arXiv:1812.01781 · astro-ph.GA, astro-ph.CO, physics.flu-dyn · Submitted 2018-12-05 · Read on arXiv

astro-ph.GA, astro-ph.CO, physics.flu-dyn

Submitted: 2018-12-05

Updated: 2018-12-05

Comments: Accepted by MNRAS

DOI: 10.1093/mnras/sty3035

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Probability Distribution Function — 3× in this paper
• Clustering — 1× in this paper · explained in 2 episodes
• Stellar Feedback — 1× in this paper · explained in 2 episodes

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