The Parameter Space Occupied by Galaxies: The Optical Window
| dc.creator | Driver, Simon P. | |
| dc.creator | Cross, Nicholas | |
| dc.date | 2000-04-14 | |
| dc.date.accessioned | 2026-07-07T01:53:09Z | |
| dc.date.available | 2026-07-07T01:53:09Z | |
| dc.description | We discuss the optical parameter space (luminosity and surface brightness) over which galaxies are known to exist and report on the results from three recent datasets: the Two-degree Field Galaxy Redshift Survey, the Hubble Deep Field north, and the Local Group. These data are combined to provide a unique and comprehensive insight into the luminosity distribution of galaxies over the range -24 < M(B) < -8 mags, and the surface brightness distribution over the range 18 < SB(Effective) < 28 mags/sq arcsec. The main conclusions are: (1) luminous low surface brightness galaxies are rare; (2) there exists a universal luminosity-surface brightness relation; (3) the most numerous galaxies are low luminosity low surface brightness dwarfs. | |
| dc.description | Review contribution for Mapping the Hidden Universe (Eds Kraan Korteweg, Henning and Andernach) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0004201 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0004201 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/864 | |
| dc.subject | Astrophysics | |
| dc.title | The Parameter Space Occupied by Galaxies: The Optical Window | |
| dc.type | text |