Resumen
In this chapter we use the method of Smoothed Particle Hydrodynamics (SPH) to study the number and properties of accretion centres formed when a molecular gas cloud collapses, starting with initial conditions corresponding either to a turbulent or a rigidly rotating sphere. To do so we use a modified version of the SPH code GADGET-2, which is capable to detect when a gas particle becomes an accretion centre, inheriting the mass and momentum of all its closest neighbours. For both types of models (turbulent and uniformly rotating), we also study the effects of considering two different initial mass distributions: a uniform-density and a centrally condensed Plummer profile. We find that the turbulent models are more propense to fragment into a larger number of protostellar objects than the purely rotating clouds. However, in both types of models the average protostellar mass increases with increasing size of the kinetic energy content of the cloud.
Idioma original | Inglés |
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Título de la publicación alojada | Computational and Experimental Fluid Mechanics with Applications to Physics, Engineering and the Environment, FLUIDOS 2012 |
Editores | Leonardo Di G. Sigalotti, Eloy Sira, Jaime Klapp |
Editorial | Springer |
Páginas | 509-520 |
Número de páginas | 12 |
ISBN (versión impresa) | 9783319001906 |
DOI | |
Estado | Publicada - 2014 |
Evento | 1st Workshop of the Venezuelan Society of Fluid Mechanics , FLUIDOS 2012 - Margarita Island, República Bolivariana de Venezuela Duración: 5 nov. 2012 → 9 nov. 2012 |
Serie de la publicación
Nombre | Environmental Science and Engineering |
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ISSN (versión impresa) | 1863-5520 |
ISSN (versión digital) | 1863-5539 |
Conferencia
Conferencia | 1st Workshop of the Venezuelan Society of Fluid Mechanics , FLUIDOS 2012 |
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País/Territorio | República Bolivariana de Venezuela |
Ciudad | Margarita Island |
Período | 5/11/12 → 9/11/12 |
Nota bibliográfica
Publisher Copyright:© Springer International Publishing Switzerland 2014.