Spectra of Cluster Galaxies at z~0.4
| dc.creator | Poggianti, Bianca M. | |
| dc.date | 1997-12-02 | |
| dc.date.accessioned | 2026-07-07T02:25:27Z | |
| dc.date.available | 2026-07-07T02:25:27Z | |
| dc.description | The ``MORPHS'' group has obtained an extensive spectroscopic dataset of galaxies in the fields of 10 rich clusters at $0.37<z<0.56$; the stellar population properties of about 700 objects have been determined from a detailed analysis of spectral line strenghts and colours, up to a galactic absolute magnitude $M_V=-20.3$ mag. Morphological informations for a consistent fraction of our sample have been previously derived from deep images of the central regions of these clusters taken with the WFPC-2 on board the HST. Spectral and morphological features can be compared in order to study the star formation histories of the different galactic types in clusters; here we show some preliminary results of this comparison. | |
| dc.description | 4 pages, uses the Latex paspconf.sty, proceedings paper of the Rome meeting "The Young Universe", Rome 29 Sep/ 3 Oct 1997 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9712034 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9712034 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11883 | |
| dc.subject | Astrophysics | |
| dc.title | Spectra of Cluster Galaxies at z~0.4 | |
| dc.type | text |