Deciphering the last major invasion of the Milky Way

Gerard Gilmore*, Rosemary F.G. Wyse, John E. Norris

*Corresponding author for this work

    Research output: Contribution to journalReview articlepeer-review

    164 Citations (Scopus)

    Abstract

    We present first results from a spectroscopic survey of ∼2000 F/G stars 0.5-5 kpc from the Galactic plane, obtained with the Two Degree Field facility on the Anglo-Australian Telescope. These data show the mean rotation velocity of the thick disk about the Galactic center a few kiloparsecs from the plane is very different than expected, being ∼100 km s-1 rather than the predicted ∼180 km s-1. We propose that our sample is dominated by stars from a disrupted satellite that merged with the disk of the Milky Way some 10-12 Gyr ago. We do not find evidence for the many substantial mergers expected in hierarchical clustering theories. We find yet more evidence that the stellar halo retains kinematic substructure, indicative of minor mergers.

    Original languageEnglish
    Pages (from-to)L39-L42
    JournalAstrophysical Journal
    Volume574
    Issue number1 II
    DOIs
    Publication statusPublished - 20 Jul 2002

    Fingerprint

    Dive into the research topics of 'Deciphering the last major invasion of the Milky Way'. Together they form a unique fingerprint.

    Cite this