Chaotic dispersal of tidal debris

Adrian M. Price-Whelan, Kathryn V. Johnston, Monica Valluri, Sarah Pearson, Andreas H W Küpper, David W. Hogg

    Research output: Contribution to journalArticle

    Abstract

    Several long, dynamically cold stellar streams have been observed around the Milky Way Galaxy, presumably formed from the tidal disruption of globular clusters. In integrable potentials - where all orbits are regular - tidal debris phase-mixes close to the orbit of the progenitor system. However, the Milky Way's dark matter halo is expected not to be fully integrable; an appreciable fraction of orbits will be chaotic. This paper examines the influence of chaos on the phase-space morphology of cold tidal streams. Streams even in weakly chaotic regions look very different from those in regular regions.We find that streams can be sensitive to chaos on a much shorter time-scale than any standard prediction (from the Lyapunov or frequency-diffusion times). For example, on a weakly chaotic orbit with a chaotic time-scale predicted to be >1000 orbital periods (>1000 Gyr), the resulting stellar stream is, after just a few 10's of orbits, substantially more diffuse than any formed on a nearby but regular orbit. We find that the enhanced diffusion of the stream stars can be understood by looking at the variance in orbital frequencies of orbit ensembles centred around the parent (progenitor) orbit. Our results suggest that long, cold streams around our Galaxy must exist only on regular (or very nearly regular) orbits; they potentially provide a map of the regular regions of the Milky Way potential. This suggests a promising new direction for the use of tidal streams to constrain the distribution of dark matter around our Galaxy.

    Original languageEnglish (US)
    Pages (from-to)1079-1098
    Number of pages20
    JournalMonthly Notices of the Royal Astronomical Society
    Volume455
    Issue number1
    DOIs
    StatePublished - 2016

    Fingerprint

    debris
    orbits
    chaotic dynamics
    chaos
    dark matter
    timescale
    Milky Way Galaxy
    galaxies
    orbitals
    globular clusters
    halos
    stars
    prediction
    predictions
    cold

    Keywords

    • Chaos
    • Dark matter
    • Galaxies
    • Galaxies
    • Galaxies
    • Galaxy
    • General
    • Halo
    • Haloes
    • Kinematics and dynamics
    • Star clusters

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Price-Whelan, A. M., Johnston, K. V., Valluri, M., Pearson, S., Küpper, A. H. W., & Hogg, D. W. (2016). Chaotic dispersal of tidal debris. Monthly Notices of the Royal Astronomical Society, 455(1), 1079-1098. https://doi.org/10.1093/mnras/stv2383

    Chaotic dispersal of tidal debris. / Price-Whelan, Adrian M.; Johnston, Kathryn V.; Valluri, Monica; Pearson, Sarah; Küpper, Andreas H W; Hogg, David W.

    In: Monthly Notices of the Royal Astronomical Society, Vol. 455, No. 1, 2016, p. 1079-1098.

    Research output: Contribution to journalArticle

    Price-Whelan, AM, Johnston, KV, Valluri, M, Pearson, S, Küpper, AHW & Hogg, DW 2016, 'Chaotic dispersal of tidal debris', Monthly Notices of the Royal Astronomical Society, vol. 455, no. 1, pp. 1079-1098. https://doi.org/10.1093/mnras/stv2383
    Price-Whelan AM, Johnston KV, Valluri M, Pearson S, Küpper AHW, Hogg DW. Chaotic dispersal of tidal debris. Monthly Notices of the Royal Astronomical Society. 2016;455(1):1079-1098. https://doi.org/10.1093/mnras/stv2383
    Price-Whelan, Adrian M. ; Johnston, Kathryn V. ; Valluri, Monica ; Pearson, Sarah ; Küpper, Andreas H W ; Hogg, David W. / Chaotic dispersal of tidal debris. In: Monthly Notices of the Royal Astronomical Society. 2016 ; Vol. 455, No. 1. pp. 1079-1098.
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