On the thick disk rotation-metallicity correlation

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Where do stars come from? T = 5 Gyr 8 kpc < R
Comparison with SDSS-GSC II Catalog data Velocity distribution model data Simulated distribution of azimuthal Velocity vs. radial velocity from <strong>the</strong> barred Disk model: 8kpc
Page 1 and 2: On the thick disk rotation-metallic
Page 3 and 4: Outline • Introduction • Proble
Page 5 and 6: Age-metallicity relation As indicat
Page 7 and 8: The origin of the Thick disk? Heati
Page 9 and 10: Radial migration in spirals • Sta
Page 11 and 12: A&A 510, L4 (2010) 40-50 km/s/dex
Page 13 and 14: Thick disk kinematic-metallicity co
Page 15 and 16: New observational results on the re
Page 17 and 18: «Old» observational results on th
Page 19: Disentangling chemistry from dynami
Page 23 and 24: Evolution of the chemical gradients
Page 25 and 26: Two infall model: inside-out disk f
Page 27 and 28: Barred disk simulation (t=5 Gyr) 10
Page 29: Conclusions • We have detected a

On the thick disk rotation-metallicity correlation

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