On the universality of the type-dependent luminosity functions
| dc.creator | Andreon, S. | |
| dc.date | 1998-04-03 | |
| dc.date.accessioned | 2026-07-07T02:26:31Z | |
| dc.date.available | 2026-07-07T02:26:31Z | |
| dc.description | We find that the bright part (M_B<-18.5 mag) of luminosity function of each Hubble type has the same shape in three poor clusters (Virgo, Fornax and Centaurus) and in two rich clusters (Coma and Cl0939+4713). The fact that these type-dependent luminosity functions are invariant in shape from poor to rich environments gives support to the hypothesis that they may be universal. We also present in tabular form improved type-dependent luminosity functions, based on a much larger sample than previous works. | |
| dc.description | A&A, in press | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9804028 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9804028 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12306 | |
| dc.subject | Astrophysics | |
| dc.title | On the universality of the type-dependent luminosity functions | |
| dc.type | text |