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Authordc.contributor.authorEscala Astorquiza, Andrés 
Authordc.contributor.authorBecerra, Fernando es_CL
Authordc.contributor.authorDel Valle, Fernando es_CL
Authordc.contributor.authorCastillo, Esteban es_CL
Admission datedc.date.accessioned2014-01-29T15:40:16Z
Available datedc.date.available2014-01-29T15:40:16Z
Publication datedc.date.issued2013-06-20
Cita de ítemdc.identifier.citationThe Astrophysical Journal, 763:39 (7pp), 2013 January 20en_US
Identifierdc.identifier.otherDOI: 10.1088/0004-637X/763/1/39
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/126325
General notedc.descriptionArtículo de publicación ISI.en_US
Abstractdc.description.abstractWe study the gravitational stability of gaseous streams in the complex environment of a galaxy merger, because mergers are known to be places of ongoing massive cluster formation and bursts of star formation. We find an analytic stability parameter for the case of gaseous streams orbiting around the merger remnant. We test our stability criterion using hydrodynamic simulations of galaxy mergers and obtain satisfactory results. We find that our criterion successfully predicts the streams that will be gravitationally unstable to fragmentation into clumps.en_US
Patrocinadordc.description.sponsorshipA.E. acknowledges partial support from the Center for Astrophysics and Associated Technologies CATA (PFB 06) and Anillo de Ciencia y Tecnolog´ıa ACT1101. F.B. and L.d.V. acknowledge support from Programa Nacional de Becas de Postgrado (Grant D-22100632 and Grant D-21090518). The simulations were performed using the HPC clusters Markarian (FONDECYT 11090216), Geryon (PFB 06), and Levque (ECM-02).en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP PUBLISHING LTDen_US
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectgalaxies: formationen_US
Títulodc.titleGRAVITATIONAL FRAGMENTATION IN GALAXY MERGERS: A STABILITY CRITERIONen_US
Document typedc.typeArtículo de revista


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile