The stellar populations of de galaxies in nearby groups

G. S. Da Costa*

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    6 Citations (Scopus)

    Abstract

    In this contribution Gemini-North NIRI J,K-observations are used to investigate the upper-Asymptotic Giant Branch (AGB) intermediate-age population in the M81 Group dwarf elliptical (dE) F8D1. Hubble Space Telescope (HST) 'snapshot' V,I-observations are also analysed to investigate the upper-AGB populations in two other M81 Group dEs, DDO 71 and kk077. In all three dEs, significant intermediate-age populations are found. Further, there are sizeable dE-to-dE differences in these populations: F8D1 contains relatively more, and relatively more luminous, upper-AGB stars. These results are compared with existing information for Local Group and Sculptor group dwarfs. It is suggested that 'environmental harrassment' plays an important role in governing dwarf galaxy evolution.

    Original languageEnglish
    Pages (from-to)366-370
    Number of pages5
    JournalPublications of the Astronomical Society of Australia
    Volume21
    Issue number4
    DOIs
    Publication statusPublished - 2004

    Fingerprint

    Dive into the research topics of 'The stellar populations of de galaxies in nearby groups'. Together they form a unique fingerprint.

    Cite this