Evolution of Normal Galaxies: HST Morphologies and Deep Spectroscopy
| dc.creator | Ellis, Richard | |
| dc.date | 1996-08-13 | |
| dc.date.accessioned | 2026-07-07T02:21:45Z | |
| dc.date.available | 2026-07-07T02:21:45Z | |
| dc.description | I review progress in understanding the evolution of normal field and cluster galaxies through the combination of HST imaging and ground-based spectroscopy. These data suggest that the bulk of the star formation producing the present-day galaxy population occurred at accessible redshifts, $z<$2. Furthermore, a surprising amount of the detailed processing that shaped the Hubble sequence and morphology-density relation occurred surprisingly recently. The stage is thus set for a concerted attack on these questions with the present generation of 8-10 metre large telescopes. An important step forward will be the development of efficient survey techniques for the systematic exploration of the $z>$1 Universe. Some possible approaches are briefly discussed. | |
| dc.description | 14 pages, Invited review for the ESO Workshop on "The Early Universe with the VLT" 1-4 April 1996, LaTeX using LAMUPHYS macro, full version with 4 B+W and 1 color figure available on ftp.ast.cam.ac.uk/public/ftp/pub/rse/eso_96.tar.gz | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9608079 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9608079 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10622 | |
| dc.subject | Astrophysics | |
| dc.title | Evolution of Normal Galaxies: HST Morphologies and Deep Spectroscopy | |
| dc.type | text |