Download | - View final version: Fossil group origins : V. The dependence of the luminosity function on the magnitude gap (PDF, 981 KiB)
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DOI | Resolve DOI: https://doi.org/10.1051/0004-6361/201425506 |
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Author | Search for: Zarattini, S.; Search for: Aguerri, J. A. L.; Search for: Sánchez-Janssen, R.1; Search for: Barrena, R.; Search for: Boschin, W.; Search for: del Burgo, C.; Search for: Castro-Rodriguez, N.; Search for: Corsini, E. M.; Search for: D’onghia, E.; Search for: Girardi, M.; Search for: Iglesias-Páramo, J.; Search for: Kundert, A.; Search for: Méndez-Abreu, J.; Search for: Vilchez, J. M. |
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Affiliation | - National Research Council of Canada. National Science Infrastructure
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Format | Text, Article |
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Subject | galaxies: clusters: general; galaxies: groups: general; galaxies: luminosity function, mass function |
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Abstract | Context. In nature we observe galaxy aggregations that span a wide range of magnitude gaps between the two first-ranked galaxies of a system (Δm₁₂). Thus, there are systems with gaps close to zero (e.g., the Coma cluster), and at the other extreme of the distribution, the largest gaps are found among the so-called fossil systems. The observed distribution of magnitude gaps is thought to be a consequence of the orbital decay of M∗ galaxies in massive halos and the associated growth of the central object. As a result, to first order the amplitude of this gap is a good statistical proxy for the dynamical age of a system of galaxies. Fossil and non-fossil systems could therefore have different galaxy populations that should be reflected in their luminosity functions. |
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Publication date | 2015-08-26 |
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Publisher | EDP Sciences |
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In | |
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Language | English |
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Peer reviewed | Yes |
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NPARC number | 23001089 |
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Export citation | Export as RIS |
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Report a correction | Report a correction (opens in a new tab) |
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Record identifier | ab93039f-465d-4a60-b1a0-e8b2d8a4638d |
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Record created | 2016-12-12 |
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Record modified | 2021-04-26 |
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