Physical effects of gas envelopes with different extension on the collapse of a gas core

In this paper we study the gravitational collapse of a molecular hydrogen gas cloud composed of a core plus a gas envelope surrounding the core. We numerically simulate the collapse of four cloud models to obtain a glimpse into the time evolution of several dynamic variables, such as the angular momentum and the aem ratio, as well as the ratios between the thermal and rotational energies with respect to the potential gravitational energy, denoted as α and β, respectively, among others. We reconsider the models introduced by Arreaga et al. (2010) in the present paper in order to produce different outcomes of the collapsing cloud characterized in terms of the aforementioned dynamical variables. Such characterization was missing in the paper by Arreaga et al. (2010), and here we show that the gas envelope extension effects on the collapsing core can be quantitatively compared.

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Main Authors: Arreaga-García,Guillermo, Saucedo Morales,Julio
Format: Digital revista
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Astronomía 2012
Online Access:http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012012000100006
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spelling oai:scielo:S0185-110120120001000062013-05-28Physical effects of gas envelopes with different extension on the collapse of a gas coreArreaga-García,GuillermoSaucedo Morales,Julio binaries/close hydrodynamics methods/numerical stars/formation In this paper we study the gravitational collapse of a molecular hydrogen gas cloud composed of a core plus a gas envelope surrounding the core. We numerically simulate the collapse of four cloud models to obtain a glimpse into the time evolution of several dynamic variables, such as the angular momentum and the aem ratio, as well as the ratios between the thermal and rotational energies with respect to the potential gravitational energy, denoted as α and β, respectively, among others. We reconsider the models introduced by Arreaga et al. (2010) in the present paper in order to produce different outcomes of the collapsing cloud characterized in terms of the aforementioned dynamical variables. Such characterization was missing in the paper by Arreaga et al. (2010), and here we show that the gas envelope extension effects on the collapsing core can be quantitatively compared.info:eu-repo/semantics/openAccessUniversidad Nacional Autónoma de México, Instituto de AstronomíaRevista mexicana de astronomía y astrofísica v.48 n.1 20122012-04-01info:eu-repo/semantics/articletext/htmlhttp://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012012000100006en
institution SCIELO
collection OJS
country México
countrycode MX
component Revista
access En linea
databasecode rev-scielo-mx
tag revista
region America del Norte
libraryname SciELO
language English
format Digital
author Arreaga-García,Guillermo
Saucedo Morales,Julio
spellingShingle Arreaga-García,Guillermo
Saucedo Morales,Julio
Physical effects of gas envelopes with different extension on the collapse of a gas core
author_facet Arreaga-García,Guillermo
Saucedo Morales,Julio
author_sort Arreaga-García,Guillermo
title Physical effects of gas envelopes with different extension on the collapse of a gas core
title_short Physical effects of gas envelopes with different extension on the collapse of a gas core
title_full Physical effects of gas envelopes with different extension on the collapse of a gas core
title_fullStr Physical effects of gas envelopes with different extension on the collapse of a gas core
title_full_unstemmed Physical effects of gas envelopes with different extension on the collapse of a gas core
title_sort physical effects of gas envelopes with different extension on the collapse of a gas core
description In this paper we study the gravitational collapse of a molecular hydrogen gas cloud composed of a core plus a gas envelope surrounding the core. We numerically simulate the collapse of four cloud models to obtain a glimpse into the time evolution of several dynamic variables, such as the angular momentum and the aem ratio, as well as the ratios between the thermal and rotational energies with respect to the potential gravitational energy, denoted as α and β, respectively, among others. We reconsider the models introduced by Arreaga et al. (2010) in the present paper in order to produce different outcomes of the collapsing cloud characterized in terms of the aforementioned dynamical variables. Such characterization was missing in the paper by Arreaga et al. (2010), and here we show that the gas envelope extension effects on the collapsing core can be quantitatively compared.
publisher Universidad Nacional Autónoma de México, Instituto de Astronomía
publishDate 2012
url http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012012000100006
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