Milky way mass and potential recovery using tidal streams in a realistic halo

Ana Bonaca, Marla Geha, Andreas H W Küpper, Jürg Diemand, Kathryn V. Johnston, David W. Hogg

    Research output: Contribution to journalArticle

    Abstract

    We present a new method for determining the Galactic gravitational potential based on forward modeling of tidal stellar streams. We use this method to test the performance of smooth and static analytic potentials in representing realistic dark matter halos, which have substructure and are continually evolving by accretion. Our FAST-FORWARD method uses a Markov Chain Monte Carlo algorithm to compare, in six-dimensional phase space, an "observed" stream to models created in trial analytic potentials. We analyze a large sample of streams that evolved in the Via Lactea II (VL2) simulation, which represents a realistic Galactic halo potential. The recovered potential parameters are in agreement with the best fit to the global, present-day VL2 potential. However, merely assuming an analytic potential limits the dark matter halo mass measurement to an accuracy of 5%-20%, depending on the choice of analytic parameterization. Collectively, the mass estimates using streams from our sample reach this fundamental limit, but individually they can be highly biased. Individual streams can both under- and overestimate the mass, and the bias is progressively worse for those with smaller perigalacticons, motivating the search for tidal streams at galactocentric distances larger than 70 kpc. We estimate that the assumption of a static and smooth dark matter potential in modeling of the GD-1- and Pal5-like streams introduces an error of up to 50% in the Milky Way mass estimates.

    Original languageEnglish (US)
    Article number94
    JournalAstrophysical Journal
    Volume795
    Issue number1
    DOIs
    StatePublished - Nov 1 2014

    Fingerprint

    halos
    recovery
    dark matter
    estimates
    galactic halos
    Markov chains
    forward modeling
    Markov chain
    substructures
    parameterization
    gravitational fields
    accretion
    modeling
    simulation
    method

    Keywords

    • dark matter
    • Galaxy: halo
    • Galaxy: structure

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Bonaca, A., Geha, M., Küpper, A. H. W., Diemand, J., Johnston, K. V., & Hogg, D. W. (2014). Milky way mass and potential recovery using tidal streams in a realistic halo. Astrophysical Journal, 795(1), [94]. https://doi.org/10.1088/0004-637X/795/1/94

    Milky way mass and potential recovery using tidal streams in a realistic halo. / Bonaca, Ana; Geha, Marla; Küpper, Andreas H W; Diemand, Jürg; Johnston, Kathryn V.; Hogg, David W.

    In: Astrophysical Journal, Vol. 795, No. 1, 94, 01.11.2014.

    Research output: Contribution to journalArticle

    Bonaca, A, Geha, M, Küpper, AHW, Diemand, J, Johnston, KV & Hogg, DW 2014, 'Milky way mass and potential recovery using tidal streams in a realistic halo', Astrophysical Journal, vol. 795, no. 1, 94. https://doi.org/10.1088/0004-637X/795/1/94
    Bonaca, Ana ; Geha, Marla ; Küpper, Andreas H W ; Diemand, Jürg ; Johnston, Kathryn V. ; Hogg, David W. / Milky way mass and potential recovery using tidal streams in a realistic halo. In: Astrophysical Journal. 2014 ; Vol. 795, No. 1.
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