A Sample of Field Ellipticals
arXiv:astro-ph/0311599 · doi:10.1086/425890
Abstract
Using well-defined selection criteria applied to the LEDA galaxy catalogue we have constructed a sample of elliptical galaxies that can be taken to lie in the field. Such criteria can easily be applied to theoretical simulations for direct comparison with observations. The variation of the number of `isolated' ellipticals with selection criteria is also investigated. A preliminary study of the environment of the field ellipticals shows that, in the mean, they are surrounded by a population of dwarf galaxies, out to projected radii of at least 500 kpc, with a radial density profile of and a luminosity function slope of . The results are compared and contrasted to the satellite population around isolated spiral galaxies.
12 pages including 3 figures and 1 table, aastex preprint style, submitted to ApJ
References in corpus (8)
- The 2dF Galaxy Redshift Survey: The b_J-band galaxy luminosity function and survey selection function
- The evolution of field early-type galaxies to z~0.7
- Early-type galaxies in low-density environments
- The Properties of Field Elliptical Galaxies at Intermediate Redshift. I: Empirical Scaling Laws
- The properties of field elliptical galaxies at intermediate redshift. II: photometry and spectroscopy of an HST selected sample
- Do clusters contain a large population of dwarf galaxies?
- The redshift-space two-point correlation functions of galaxies and groups in the Nearby Optical Galaxy sample
- The Global, Local and Cluster Galaxy Luminosity Function
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- Isolated elliptical galaxies and their globular cluster systems. II. NGC 7796 - globular clusters, dynamics, companion
- The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
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