Interpreting the relationship between galaxy luminosity, color, and environment

Andreas A. Berlind, Michael R. Blanton, David W. Hogg, David H. Weinberg, Romeel Davé, Daniel J. Eisenstein, Neal Katz

    Research output: Contribution to journalArticle

    Abstract

    We study the relationship between galaxy luminosity, color, and environment in a cosmological simulation of galaxy formation. Using a simple prescription to assign colors and luminosities to simulated galaxies, we compare the predicted relationship with that observed for SDSS galaxies and find that the model successfully predicts most of the qualitative features seen in the data, but also shows some interesting differences. Specifically, the simulation predicts that the local density around bright red galaxies is a strong increasing function of luminosity, but does not depend much on color at fixed luminosity. Moreover, we show that these trends are due to central galaxies in dark matter halos whose baryonic masses correlate strongly with halo mass. The simulation also predicts that the local density around blue galaxies is a strong increasing function of color, but does not depend much on luminosity at fixed color. We show that these trends are due to satellite galaxies in halos whose stellar ages correlate with halo mass. Finally, the simulation fails to predict the luminosity dependence of environments observed around low-luminosity red galaxies. However, we show that this is most likely due to the simulation's limited resolution. A study of a higher resolution, smaller volume simulation suggests that this dependence is caused by the fact that all low-luminosity red galaxies are satellites in massive halos, whereas intermediate-luminosity red galaxies are a mixture of satellites in massive halos, and central galaxies in less massive halos.

    Original languageEnglish (US)
    Pages (from-to)625-632
    Number of pages8
    JournalAstrophysical Journal
    Volume629
    Issue number2 I
    DOIs
    StatePublished - Aug 20 2005

    Fingerprint

    luminosity
    galaxies
    color
    halos
    simulation
    trends
    galactic evolution
    dark matter
    high resolution

    Keywords

    • Cosmology: theory
    • Galaxies: formation
    • Large-scale structure of universe

    ASJC Scopus subject areas

    • Space and Planetary Science

    Cite this

    Berlind, A. A., Blanton, M. R., Hogg, D. W., Weinberg, D. H., Davé, R., Eisenstein, D. J., & Katz, N. (2005). Interpreting the relationship between galaxy luminosity, color, and environment. Astrophysical Journal, 629(2 I), 625-632. https://doi.org/10.1086/431658

    Interpreting the relationship between galaxy luminosity, color, and environment. / Berlind, Andreas A.; Blanton, Michael R.; Hogg, David W.; Weinberg, David H.; Davé, Romeel; Eisenstein, Daniel J.; Katz, Neal.

    In: Astrophysical Journal, Vol. 629, No. 2 I, 20.08.2005, p. 625-632.

    Research output: Contribution to journalArticle

    Berlind, AA, Blanton, MR, Hogg, DW, Weinberg, DH, Davé, R, Eisenstein, DJ & Katz, N 2005, 'Interpreting the relationship between galaxy luminosity, color, and environment', Astrophysical Journal, vol. 629, no. 2 I, pp. 625-632. https://doi.org/10.1086/431658
    Berlind AA, Blanton MR, Hogg DW, Weinberg DH, Davé R, Eisenstein DJ et al. Interpreting the relationship between galaxy luminosity, color, and environment. Astrophysical Journal. 2005 Aug 20;629(2 I):625-632. https://doi.org/10.1086/431658
    Berlind, Andreas A. ; Blanton, Michael R. ; Hogg, David W. ; Weinberg, David H. ; Davé, Romeel ; Eisenstein, Daniel J. ; Katz, Neal. / Interpreting the relationship between galaxy luminosity, color, and environment. In: Astrophysical Journal. 2005 ; Vol. 629, No. 2 I. pp. 625-632.
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