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The elliptical galaxy colour-magnitude relation as a discriminant between the monolithic and merger paradigms

Kaviraj, S. ; Devriendt, J. E. G. ; Ferreras, I. ; Yi, S. K.

In: Monthly Notices of the Royal Astronomical Society, 2005, vol. 360, no. 1, p. 60-68

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    Titre
    • The elliptical galaxy colour-magnitude relation as a discriminant between the monolithic and merger paradigms
    Auteur
    • Kaviraj, S.. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
    • Devriendt, J. E. G.. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
    • Ferreras, I.. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
    • Yi, S. K.. Department of Physics, University of Oxford, Keble Road, Oxford OX1 3RH
    Type de document
    • Postprint
    Langue
    • Anglais
    Publié dans
    • Monthly Notices of the Royal Astronomical Society, 2005, vol. 360, no. 1, p. 60-68. Blackwell Science Ltd
    Autre version électronique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:301510
    Summary
    The colour-magnitude relation (CMR) of cluster elliptical galaxies has been widely used to constrain their star formation histories (SFHs) and to discriminate between the monolithic collapse and merger paradigms of elliptical galaxy formation. We use a Λ cold dark matter hierarchical merger model of galaxy formation to investigate the existence and redshift evolution of the elliptical galaxy CMR in the merger paradigm. We show that the SFH of cluster ellipticals predicted by the model is quasi-monolithic, with only ∼10 per cent of the total stellar mass forming after z∼ 1. The quasi-monolithic SFH results in a predicted CMR that agrees well with its observed counterpart in the redshift range 0 < z < 1.27. We use our analysis to argue that the elliptical-only CMR can be used to constrain the SFHs of present-day cluster ellipticals only if we believe a priori in the monolithic collapse model. It is not a meaningful tool for constraining the SFH in the merger paradigm, since a progressively larger fraction of the progenitor set of present-day cluster ellipticals is contained in late-type star-forming systems at higher redshift, which cannot be ignored when deriving the SFHs. Hence, the elliptical-only CMR is not a useful discriminant between the two competing theories of elliptical galaxy evolution