the galaxy as seen by rave

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The Galaxy as seen by RAVE L. Veltz, O. Bienaymé & A. Just

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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. - PowerPoint PPT Presentation

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Page 1: The Galaxy as seen by RAVE

The Galaxy as seen by RAVE

L. Veltz, O. Bienaymé & A. Just

Page 2: The Galaxy as seen by RAVE

Outline Model Observations Structure Kinematics Metallicity

Page 3: The Galaxy as seen by RAVE

Model Cigal

Page 4: The Galaxy as seen by RAVE

i => isothermal components

k => absolute magnitudes

Equation of stellar statistics:

Our modelOur model

Page 5: The Galaxy as seen by RAVE

Gravitation

alPotential

density distribution

velocitydispersion

Φ(z) = 2πG Σ0( z2 + D2 −D) + ρ eff z2

( )

Vertical gravitational potential:

self-consistentself-consistent

Page 6: The Galaxy as seen by RAVE

The analysis of the Galactic Disk structure relies on:

• Star counts

• Proper motions

• Radial velocities

2massComplete within

5 to 15.4 magnitudes

UCAC23 to 7 mas.y-1

within 6 to 14 magnitudes

RAVEInternal error of 2 km.s-1

Our samples Our samples

Page 7: The Galaxy as seen by RAVE

Fit the observations

Count Radial velocity

Proper motions

Page 8: The Galaxy as seen by RAVE

Kinematics distribution function

Thin disk Thic

k disk

Page 9: The Galaxy as seen by RAVE

Dwarf/Giant separation

Page 10: The Galaxy as seen by RAVE

Absolute magnitudes:

Sub-giants

MK=-0.89

MK=-0.17

Dwarfs MK=4.15

Clump giantsMK=-1.61

Color selectionColor selection

2mass-MSX-Hipparcos

Page 11: The Galaxy as seen by RAVE

HR diagram

Page 12: The Galaxy as seen by RAVE

Dwarf/Giant separation

Giants Dwarfs

Subgiants

Page 13: The Galaxy as seen by RAVE

Selection of dwarfs

Page 14: The Galaxy as seen by RAVE

Giants

Dwarfs

Subgiants

Dwarf/Giant separation

Page 15: The Galaxy as seen by RAVE

Dwarf/Giant separation

Giants Dwarfs

Subgiants

Page 16: The Galaxy as seen by RAVE

Dwarf/Giant separation

Giants Subgiants Dwarfs

Page 17: The Galaxy as seen by RAVE

hyp.: all stars are Dwarfs

Photometric distance

Page 18: The Galaxy as seen by RAVE

Observations versus Model

Thin/thick disk

transition

Thick disk

45 Km/s

Thin disk

15-20 Km/s

photometric distance (pc)

Page 19: The Galaxy as seen by RAVE

Scaleheight

Page 20: The Galaxy as seen by RAVE

Scale-height

Thin disk

Thick disk

Thin disk:

hz=225 ± 10 pc

Thick disk:

hz=1048 ± 36 pc

thick/

thin=8%

Page 21: The Galaxy as seen by RAVE

Scalelength

Page 22: The Galaxy as seen by RAVE

hR=2500pc

Page 23: The Galaxy as seen by RAVE

hR,1=1800pc & hR,2=2800pc

Page 24: The Galaxy as seen by RAVE

Kinematics

Page 25: The Galaxy as seen by RAVE

Selection of dwarfs

Page 26: The Galaxy as seen by RAVE

Selection of dwarfs

Page 27: The Galaxy as seen by RAVE

Selection of dwarfs

Page 28: The Galaxy as seen by RAVE

Selection of dwarfs

Page 29: The Galaxy as seen by RAVE

Dispersion-color

Page 30: The Galaxy as seen by RAVE

Dispersion-color

Page 31: The Galaxy as seen by RAVE

B-V <=> J-K

Page 32: The Galaxy as seen by RAVE
Page 33: The Galaxy as seen by RAVE

Dispersion-color

Page 34: The Galaxy as seen by RAVE

Dispersion - color

Page 35: The Galaxy as seen by RAVE

Dispersion vs distance

Page 36: The Galaxy as seen by RAVE

sigW-col (distance)

Page 37: The Galaxy as seen by RAVE

Metallicity

Page 38: The Galaxy as seen by RAVE

SDSS - RAVE

Page 39: The Galaxy as seen by RAVE

Metallicity

Page 40: The Galaxy as seen by RAVE

Metallicity-dispersion

Page 41: The Galaxy as seen by RAVE

Conclusions

Page 42: The Galaxy as seen by RAVE

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