Identification and Morphologies of Galaxies with Old Stellar Populations at z ~ 2.5

Simple item page
dc.creatorStockton, Alan
dc.creatorMcGrath, Elizabeth
dc.date2007-02-05
dc.date.accessioned2026-07-07T07:44:34Z
dc.date.available2026-07-07T07:44:34Z
dc.descriptionWe describe a study of morphologies of galaxies with old stellar populations in radio-source fields at z ~ 2.5. A significant fraction of these are dominated by disks of old stars, and none we have found so far has the properties of present-epoch ellipticals. Recent Spitzer IRAC data confirms that at least one of our prime examples is definitely not a reddened star-forming galaxy.
dc.descriptionTo be published in the proceedings of the Durham "Cosmic Frontiers" conference, held in August, 2006 (ASP Conference Series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0702130
dc.identifierhttp://arxiv.org/abs/astro-ph/0702130
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123247
dc.subjectAstrophysics
dc.titleIdentification and Morphologies of Galaxies with Old Stellar Populations at z ~ 2.5
dc.typetext

Files

Collections

arXiv