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THE EFFECTS ON A CORE COLLAPSE OF CHANGES IN THE NUMBER AND SIZE OF TURBULENT MODES OF VELOCITY

We consider 28 particle-based simulations aimed at comparing the gravitational collapse of a spherically symmetric, uniform gas core in which two extreme types of turbulent spectra of velocity have been initially induced, so that ∇· ~v = 0 (14 simulations) and ∇×~v = 0 (14 simulations). For all the...

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Veröffentlicht in:Revista Mexicana de Astronomía y Astrofísica
1. Verfasser: Guillermo Arreaga-García
Format: Artigo
Sprache:Inglês
Veröffentlicht: Universidad Nacional Autónoma de México 2017
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Online-Zugang:https://www.redalyc.org/articulo.oa?id=57153206027
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