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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Format: | Article |
Language: | English |
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Astronomical Observatory, Department of Astronomy, Belgrade
2007-01-01
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Series: | Serbian Astronomical Journal |
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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. . |
first_indexed | 2024-12-11T22:40:57Z |
format | Article |
id | doaj.art-0c21d61f5b0a41b587547e39cab0c35e |
institution | Directory Open Access Journal |
issn | 1450-698X 1820-9289 |
language | English |
last_indexed | 2024-12-11T22:40:57Z |
publishDate | 2007-01-01 |
publisher | Astronomical Observatory, Department of Astronomy, Belgrade |
record_format | Article |
series | Serbian Astronomical Journal |
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 |