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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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autor: | |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2017
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57153206027 |
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