Modeling the Milky Way disk dynamics
Modeling the Milky Way disk dynamics
Modeling the Milky Way disk dynamics
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RAVE sample• multi-fiber spectroscopic survey•DR3 (Siebert et al. 2012): 500000 spectra•Proper motions: UCAC2, PPMX•Spectro-photometric distances: Burnett & Binney 2010•6D phase space for 2·10 5 stars•6D phase space for 10 5 stars•|Z| ≤ 300 pc• Our goal: velocity distribution at different positions• Regional Standard of Rest (McMillan & Binney 2010):R☉=7.8 kpc, v☉=247 km/s , U☉=10 km/s, V☉=11 km/sT. Antoja Sydney, 24/07/2012