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The Galaxy as seen by RAVE. L. Veltz, O. Bienaymé & A. Just. Outline. Model Observations Structure Kinematics Metallicity. Model Cigal. Our model. Equation of stellar statistics:. i => isothermal components. k => absolute magnitudes. self-consistent. Gravitational Potential.
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The Galaxy as seen by RAVE L. Veltz, O. Bienaymé & A. Just
Outline Model Observations Structure Kinematics Metallicity
Our model Equation of stellar statistics: i => isothermal components k => absolute magnitudes
self-consistent Gravitational Potential density distribution velocity dispersion Vertical gravitational potential:
UCAC2 RAVE 2mass Complete within 5 to 15.4 magnitudes 3 to 7 mas.y-1 within 6 to 14 magnitudes Internal error of 2 km.s-1 Our samples • The analysis of the Galactic Disk structure relies on: • Star counts • Proper motions • Radial velocities
Fit the observations Count Radial velocity Proper motions
Kinematics distribution function Thin disk Thick disk
Color selection Absolute magnitudes: Clump giants MK=-1.61 Sub-giants MK=-0.89 MK=-0.17 Dwarfs MK=4.15 2mass-MSX-Hipparcos
Dwarf/Giant separation Subgiants Giants Dwarfs
Dwarf/Giant separation Dwarfs Giants Subgiants
Dwarf/Giant separation Dwarfs Giants Subgiants
Dwarf/Giant separation Giants Subgiants Dwarfs
Photometric distance hyp.: all stars are Dwarfs
Observations versus Model Thin/thick disk transition 45 Km/s 15-20 Km/s Thick disk Thin disk photometric distance (pc)
Scale-height Thin disk Thin disk: hz=225 ± 10 pc Thick disk: hz=1048 ± 36 pc thick/ thin=8% Thick disk
Results • Kinematical decomposition • Clear separation between the thin and the the thick disk • Separation of dwarfs/giants • Determination Scale height /length • Kinematics function of Z • Metallicity • Space • kinematics