MAPPING THE GALACTIC BULGE Manuela Zoccali

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The bulge ageThe VVV reaches the turnoff in most fields.BUT: CMD analysis needs synthesisdisk decontamination needed (5 yr baseline)good handle on reddening(+0.21,–6.28)
100 Million star CMD(Saito et al. in prep.)red clumpturnoff
Page 4 and 5: Further evidences ofa Galactic barS
Page 7 and 8: 2010s - The X-shaped bulgeNataf et
Page 9 and 10: 2010s - The X-shaped bulgeInterpret
Page 11 and 12: 2010s - The X-shaped bulgeSaito et
Page 13 and 14: The VISTAVariables in the Vía a L
Page 17 and 18: Orbits of stars in the (model) pean
Page 19 and 20: Kinematics in the X-shaped bulgeVá
Page 21 and 22: The bulge age► pure old age (~10
Page 23 and 24: The bulge metallicity distributionR
Page 25 and 26: vertex deviation (°)The bulge meta
Page 27 and 28: [ O, Mg, Si, Ca, Ti / Fe ][ O, Mg,
Page 29 and 30: The bulge metallicity distributionw
Page 31 and 32: ulge metallicity(not a) large scale
Page 33 and 34: BW calib field (HR21)link to GESbul
Page 35 and 36: ulge metallicityPI: S. Majewskiwe n
Page 38 and 39: JThe Milky Way Inner Diskdisk red c
Page 42: The bulge helium contentfrom OGLE I
Page 45: The bulge metallicity distributionH

MAPPING THE GALACTIC BULGE Manuela Zoccali

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