Mergers and star formation in SPH cosmological simulations

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dc.creatorTissera, Patricia B.
dc.date1999-11-02
dc.date.accessioned2026-07-07T02:34:10Z
dc.date.available2026-07-07T02:34:10Z
dc.descriptionThe star formation rate history of galactic objects in hydrodynamical cosmological simulations are analyzed in relation to their merger histories. The findings suggest that massive mergers produce more efficient starbursts and that, depending on the internal structure of the objects, double starbursts could also occur.
dc.description5 pages, 2 PS figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9911009
dc.identifierhttp://arxiv.org/abs/astro-ph/9911009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15141
dc.subjectAstrophysics
dc.titleMergers and star formation in SPH cosmological simulations
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