Extremely Red Galaxies: Old or Dusty ?

Simple item page
dc.creatorCimatti, Andrea
dc.creatorAndreani, Paola
dc.creatorRöttgering, Huub
dc.creatorTilanus, Remo
dc.date1998-10-01
dc.date.accessioned2026-07-07T02:28:09Z
dc.date.available2026-07-07T02:28:09Z
dc.descriptionThe nature of the extremely red galaxies is poorly known, the critical issue being whether they are old ellipticals at $z>1.5$ or distant star-forming galaxies strongly reddened by dust extinction. Here we review the little we know about them, and we present recent and preliminary results from our ongoing submillimeter -- millimeter observations.
dc.description4 pages, 1 figure. To appear in the proceedings of the Xth Rencontres de Blois: The Birth of Galaxies; Blois, France, July 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9810004
dc.identifierhttp://arxiv.org/abs/astro-ph/9810004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12999
dc.subjectAstrophysics
dc.titleExtremely Red Galaxies: Old or Dusty ?
dc.typetext

Files

Collections

arXiv