Dependence of Star Formation Rate on Overdensity

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dc.creatorNagamine, Kentaro
dc.creatorCen, Renyue
dc.creatorOstriker, Jeremiah P.
dc.date1999-12-01
dc.date2003-11-13
dc.date.accessioned2026-07-07T02:34:44Z
dc.date.available2026-07-07T02:34:44Z
dc.descriptionWe use a large-scale Lambda-CDM hydrodynamical simulation to assess the dependence of the cosmic Star Formation Rate (SFR) on overdensity of luminosity. The `morphology-density relation' is qualitatively captured when the SFR is plotted as a function of redshift, divided into the quartiles of the overdensity distribution.
dc.description2 pages, 1 figure. Proceedings of the 4th RESCEU International Symposium: "The Birth and Evolution of the Universe" (Tokyo, Japan, Nov. 16-19, 1999), p.383
dc.identifierhttps://arxiv.org/abs/astro-ph/9912023
dc.identifierhttp://arxiv.org/abs/astro-ph/9912023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15360
dc.subjectAstrophysics
dc.titleDependence of Star Formation Rate on Overdensity
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