Simulating radially outward winds within a turbulent gas clump

Guillermo Arreaga-García, Silvio Oreste Topa

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

© Springer International Publishing Switzerland 2016. By using the particle-based code Gadget2, we follow the evolution of a gas clump, in which a gravitational collapse is initially induced. The particles representing the gas clump have initially a velocity according to a turbulent spectrum built in a Fourier space of 643grid elements. In a very early stage of evolution of the clump, a set of gas particles representing the wind, suddenly move outwards from the clump’s center. We consider only two kinds of winds, namely: one with spherical symmetry and a second one being a bipolar collimated jet. In order to assess the dynamical change in the clump due to interaction with the winds, we show iso-velocity and iso-density plots for all our simulations.
Original languageAmerican English
Title of host publicationSimulating radially outward winds within a turbulent gas clump
Pages326-342
Number of pages17
ISBN (Electronic)9783319322421
DOIs
StatePublished - 1 Jan 2016
EventCommunications in Computer and Information Science -
Duration: 1 Jan 2016 → …

Publication series

NameCommunications in Computer and Information Science
Volume595
ISSN (Print)1865-0929

Conference

ConferenceCommunications in Computer and Information Science
Period1/01/16 → …

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