GRAVITATIONAL FRAGMENTATION IN GALAXY MERGERS: A STABILITY CRITERION
Author
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Escala Astorquiza, Andrés
Author
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Becerra, Fernando
es_CL
Author
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Del Valle, Fernando
es_CL
Author
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Castillo, Esteban
es_CL
Admission date
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2014-01-29T15:40:16Z
Available date
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2014-01-29T15:40:16Z
Publication date
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2013-06-20
Cita de ítem
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The Astrophysical Journal, 763:39 (7pp), 2013 January 20
en_US
Identifier
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DOI: 10.1088/0004-637X/763/1/39
Identifier
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https://repositorio.uchile.cl/handle/2250/126325
General note
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Artículo de publicación ISI.
en_US
Abstract
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We 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
Patrocinador
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A.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).