The Nearby Early-type Galaxies Survey (ENEAR): Project description and Some Preliminary Results
| dc.creator | Wegner, G. | |
| dc.creator | da Costa, L. N. | |
| dc.creator | Alonso, M. V. | |
| dc.creator | Bernardi, M. | |
| dc.creator | Wilmer, C. N. A. | |
| dc.creator | Pellegrini, P. S. | |
| dc.creator | Rite, C. | |
| dc.creator | Maia, M. | |
| dc.date | 1999-08-31 | |
| dc.date.accessioned | 2026-07-07T02:32:58Z | |
| dc.date.available | 2026-07-07T02:32:58Z | |
| dc.description | The ENEAR project is an all-sky survey of nearby early-type galaxies. About 2200 new spectra and R-band images of over 1500 galaxies together with published data were assembled into a large catalog containing over 2000 objects with cz, sigma, photometric data, and line strengths on a uniform system. From this extensive database a magnitude-limited sample has been drawn comprising ~ 1400 galaxies brighter than m_B = 14.5, cz < 7000 km/s, and type T -2 or less with measured distances (ENEARf) and about 500 early-type galaxies in 28 clusters/groups (ENEARc) to derive an internally consistent D_n-sigma relation to estimate galaxy distances. In this contribution we discuss some general properties of ENEAR and briefly describe some preliminary results. | |
| dc.description | Eight pages, including two figures. To appear in Proceedings of the Cosmic Flows Workshop, Victoria, B. C., Canada, July 1999, eds. S. Courteau, M. Strauss, and J. Willick | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9908354 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9908354 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14664 | |
| dc.subject | Astrophysics | |
| dc.title | The Nearby Early-type Galaxies Survey (ENEAR): Project description and Some Preliminary Results | |
| dc.type | text |