Local elliptical galaxies: Some aspects of theory vs. observations

In this paper we analyze on, the sample of the local elliptical galaxies, some predictions of various cosmological theories. We start with the sample of ellipticals described in Samurović (2007b) and confront the established concentration parameters and mass-to-light ratios of these objects with var...

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Main Author: Samurović S.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2007-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2007/1450-698X0775007S.pdf
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author Samurović S.
author_facet Samurović S.
author_sort Samurović S.
collection DOAJ
description In this paper we analyze on, the sample of the local elliptical galaxies, some predictions of various cosmological theories. We start with the sample of ellipticals described in Samurović (2007b) and confront the established concentration parameters and mass-to-light ratios of these objects with various cosmological models, i.e. models given by Navarro, Frank and White (NFW) (1996, 1997) and Burkert (1995), respectively. We find that the bright galaxy (NGC 5846), for which the sum α + β is high, can be reasonably modelled by the NFW models. The Burkert model provides rather good predictions of the dark matter content at one effective radius. There is an indication that bright ellipticals (MB >˜ -21.0) are more dark matter dominated that the fainter ones (MB >˜ -21.0).
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spelling doaj.art-f5fca2b9ff00471bb1abc2004dacb6952022-12-22T00:39:47ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892007-01-01200717571310.2298/SAJ0775007S1450-698X0775007SLocal elliptical galaxies: Some aspects of theory vs. observationsSamurović S.0Astronomical Observatory, BelgradeIn this paper we analyze on, the sample of the local elliptical galaxies, some predictions of various cosmological theories. We start with the sample of ellipticals described in Samurović (2007b) and confront the established concentration parameters and mass-to-light ratios of these objects with various cosmological models, i.e. models given by Navarro, Frank and White (NFW) (1996, 1997) and Burkert (1995), respectively. We find that the bright galaxy (NGC 5846), for which the sum α + β is high, can be reasonably modelled by the NFW models. The Burkert model provides rather good predictions of the dark matter content at one effective radius. There is an indication that bright ellipticals (MB >˜ -21.0) are more dark matter dominated that the fainter ones (MB >˜ -21.0).http://www.doiserbia.nb.rs/img/doi/1450-698X/2007/1450-698X0775007S.pdfgalaxies: kinematics and dynamicsgalaxies: elliptical and lenticularcDgalaxies: structuredark matter
spellingShingle Samurović S.
Local elliptical galaxies: Some aspects of theory vs. observations
Serbian Astronomical Journal
galaxies: kinematics and dynamics
galaxies: elliptical and lenticular
cD
galaxies: structure
dark matter
title Local elliptical galaxies: Some aspects of theory vs. observations
title_full Local elliptical galaxies: Some aspects of theory vs. observations
title_fullStr Local elliptical galaxies: Some aspects of theory vs. observations
title_full_unstemmed Local elliptical galaxies: Some aspects of theory vs. observations
title_short Local elliptical galaxies: Some aspects of theory vs. observations
title_sort local elliptical galaxies some aspects of theory vs observations
topic galaxies: kinematics and dynamics
galaxies: elliptical and lenticular
cD
galaxies: structure
dark matter
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2007/1450-698X0775007S.pdf
work_keys_str_mv AT samurovics localellipticalgalaxiessomeaspectsoftheoryvsobservations