A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core

This work presents three-dimensional hydrodynamical simulations with the fully parallel GAGDET2 code, to model a rotating source that emits wind in order to study the subsequent dynamics of the wind in three independent scenarios. In the first scenario we consider several models of the wind source,...

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Main Author: Guillermo Arreaga-Garcia
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2015/472490
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author Guillermo Arreaga-Garcia
author_facet Guillermo Arreaga-Garcia
author_sort Guillermo Arreaga-Garcia
collection DOAJ
description This work presents three-dimensional hydrodynamical simulations with the fully parallel GAGDET2 code, to model a rotating source that emits wind in order to study the subsequent dynamics of the wind in three independent scenarios. In the first scenario we consider several models of the wind source, which is characterized by a rotation velocity Vrot and an escape velocity Vesc, so that the models have a radially outward wind velocity magnitude Vrad given by 1, 2, 4, 6, and 8 times Vrot. In the second scenario, we study the interaction of winds emitted from a binary system in two kinds of models: one in which the source remains during the wind emission and a second one in which all the source itself becomes wind. In the third scenario we consider the interaction of a rotating source that emits wind within a collapsing and rotating core. In this scenario we consider only wind models of the second kind built over a new initial radial mesh, such that the angular velocity of the wind Ωw is 1, 100, and 1000 times the angular velocity of the core Ωc.
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spelling doaj-art-3bbf65fbb4074e2ea736c83455f6467a2025-08-20T02:08:00ZengWileyAdvances in Astronomy1687-79691687-79772015-01-01201510.1155/2015/472490472490A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating CoreGuillermo Arreaga-Garcia0Departamento de Investigación en Física, Universidad de Sonora, Apartado Postal 14740, 83000 Hermosillo, SON, MexicoThis work presents three-dimensional hydrodynamical simulations with the fully parallel GAGDET2 code, to model a rotating source that emits wind in order to study the subsequent dynamics of the wind in three independent scenarios. In the first scenario we consider several models of the wind source, which is characterized by a rotation velocity Vrot and an escape velocity Vesc, so that the models have a radially outward wind velocity magnitude Vrad given by 1, 2, 4, 6, and 8 times Vrot. In the second scenario, we study the interaction of winds emitted from a binary system in two kinds of models: one in which the source remains during the wind emission and a second one in which all the source itself becomes wind. In the third scenario we consider the interaction of a rotating source that emits wind within a collapsing and rotating core. In this scenario we consider only wind models of the second kind built over a new initial radial mesh, such that the angular velocity of the wind Ωw is 1, 100, and 1000 times the angular velocity of the core Ωc.http://dx.doi.org/10.1155/2015/472490
spellingShingle Guillermo Arreaga-Garcia
A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core
Advances in Astronomy
title A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core
title_full A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core
title_fullStr A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core
title_full_unstemmed A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core
title_short A Hydrodynamical Model of a Rotating Wind Source and Its Effects on the Collapse of a Rotating Core
title_sort hydrodynamical model of a rotating wind source and its effects on the collapse of a rotating core
url http://dx.doi.org/10.1155/2015/472490
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