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Cited by 391

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The age of elliptical galaxies and bulges in a merger model

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Kauffmann, G.·1996·Monthly Notices of the Royal Astronomical Society

Abstract

The tightness of the observed colour-magnitude and Mg$_{2}$- velocity dispersion relations for elliptical galaxies has often been cited as an argument against a picture in which ellipticals form by the merging of spiral disks. A common view is that merging would mix together stars of disparate ages and produce a large scatter in these relations. Here I use semi-analytic models of galaxy formation to derive the distribution of the mean ages, colours and metallicities of the stars in elliptical galaxies formed by mergers in a flat CDM universe. It is seen that most of the stars in ellipticals form at relatively high redshift (z > 1.9) and that the predicted scatter in the colour-magnitude and Mg_2 - sigma relations falls within observational bounds. I conclude that the apparent homogeneity in the properties of the stellar populations of ellipticals is not inconsistent with a merger scenario for the origin of these systems.

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Metadata

Authors
Kauffmann, G.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1996-07-11
Volume
281
Issue
2
Pages
487-492
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W1575728940
Cited by
391
References
1
FWCI
22.48
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The age of elliptical galaxies and bulges in a merger model. https://app.cochat.ai/papers/10.1093/mnras/281.2.487
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Kauffmann, G. (1996). The age of elliptical galaxies and bulges in a merger model. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/281.2.487

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