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A DIRECT DYNAMICAL MEASUREMENT OF THE MILKY WAY'S DISK SURFACE DENSITY PROFILE, DISK SCALE LENGTH, AND DARK MATTER PROFILE AT 4 kpc ≲ R ≲ 9 kpc
Ist Teil von
The Astrophysical journal, 2013-12, Vol.779 (2), p.1-30
Ort / Verlag
United States
Erscheinungsjahr
2013
Link zum Volltext
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
We present and apply rigorous dynamical modeling with which we infer unprecedented constraints on the stellar and dark matter mass distribution within our Milky Way (MW), based on large sets of phase-space data on individual stars. We independently fit a parameterized MW potential and a three-integral, action-based distribution function (DF) to the phase-space data of 43 separate abundance-selected sub-populations (MAPs), accounting for the complex selection effects affecting the data. Using metal-poor MAPs with small radial scale lengths as dynamical tracers probes 4.5 kpc [lap] RGC [lap] 7 kpc, while MAPs with longer radial scale lengths sample 7 kpc [lap] RGC [lap] 9 kpc. Our results show that action-based DF modeling of complex stellar data sets is now a feasible approach that will be fruitful for interpreting Gaia data.