Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio

In this paper the problem of the phenomenological modelling of elliptical galaxies using various available observational data is presented. Recently, Tortora, Cardona and Piedipalumbo (2007) suggested a double power law expression for the global cumulative mass-to-light ratio of elliptical galaxies....

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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/2007/1450-698X0774035S.pdf
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author Samurović S.
author_facet Samurović S.
author_sort Samurović S.
collection DOAJ
description In this paper the problem of the phenomenological modelling of elliptical galaxies using various available observational data is presented. Recently, Tortora, Cardona and Piedipalumbo (2007) suggested a double power law expression for the global cumulative mass-to-light ratio of elliptical galaxies. We tested their expression on a sample of ellipticals for which we have the estimates of the mass-to-light ratio beyond ~ 3 effective radii, a region where dark matter is expected to play an important dynamical role. We found that, for all the galaxies in our sample, we have α + β > 0, but that this does not necessarily mean a high dark matter content. The galaxies with higher mass (and higher dark matter content) also have higher value of α+β. It was also shown that there is an indication that the galaxies with higher value of the effective radius also have higher dark matter content. .
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spelling doaj.art-0c21d61f5b0a41b587547e39cab0c35e2022-12-22T00:47:48ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892007-01-012007174354210.2298/SAJ0774035S1450-698X0774035SPhenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratioSamurović S.0Astoronomska opservatorija, BeogradIn this paper the problem of the phenomenological modelling of elliptical galaxies using various available observational data is presented. Recently, Tortora, Cardona and Piedipalumbo (2007) suggested a double power law expression for the global cumulative mass-to-light ratio of elliptical galaxies. We tested their expression on a sample of ellipticals for which we have the estimates of the mass-to-light ratio beyond ~ 3 effective radii, a region where dark matter is expected to play an important dynamical role. We found that, for all the galaxies in our sample, we have α + β > 0, but that this does not necessarily mean a high dark matter content. The galaxies with higher mass (and higher dark matter content) also have higher value of α+β. It was also shown that there is an indication that the galaxies with higher value of the effective radius also have higher dark matter content. .http://www.doiserbia.nb.rs/img/doi/1450-698X/2007/1450-698X0774035S.pdfgalaxies: kinematics and dynamicsgalaxies: elliptical and lenticulargalaxies: structuredark mattergalaxies
spellingShingle Samurović S.
Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio
Serbian Astronomical Journal
galaxies: kinematics and dynamics
galaxies: elliptical and lenticular
galaxies: structure
dark matter
galaxies
title Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio
title_full Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio
title_fullStr Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio
title_full_unstemmed Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio
title_short Phenomenological approach to the modelling of elliptical galaxies: The problem of the mass-to-light ratio
title_sort phenomenological approach to the modelling of elliptical galaxies the problem of the mass to light ratio
topic galaxies: kinematics and dynamics
galaxies: elliptical and lenticular
galaxies: structure
dark matter
galaxies
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2007/1450-698X0774035S.pdf
work_keys_str_mv AT samurovics phenomenologicalapproachtothemodellingofellipticalgalaxiestheproblemofthemasstolightratio