Comparing accretion centres between rotating and turbulent cloud cores

Guillermo Arreaga-García*, Jaime Klapp

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

1 Scopus citations

Abstract

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.

Original languageEnglish
Title of host publicationComputational and Experimental Fluid Mechanics with Applications to Physics, Engineering and the Environment, FLUIDOS 2012
EditorsLeonardo Di G. Sigalotti, Eloy Sira, Jaime Klapp
PublisherSpringer
Pages509-520
Number of pages12
ISBN (Print)9783319001906
DOIs
StatePublished - 2014
Event1st Workshop of the Venezuelan Society of Fluid Mechanics , FLUIDOS 2012 - Margarita Island, Venezuela, Bolivarian Republic of
Duration: 5 Nov 20129 Nov 2012

Publication series

NameEnvironmental Science and Engineering
ISSN (Print)1863-5520
ISSN (Electronic)1863-5539

Conference

Conference1st Workshop of the Venezuelan Society of Fluid Mechanics , FLUIDOS 2012
Country/TerritoryVenezuela, Bolivarian Republic of
City Margarita Island
Period5/11/129/11/12

Bibliographical note

Publisher Copyright:
© Springer International Publishing Switzerland 2014.

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