Stéphane Courteau

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Ascona/Terschelling Highlights • Disk truncation is not understood yet: remains an interesting problem • Beautiful multi-wavelength high-resolution imaging – From UV (GALEX) via HST to Spitzer and HI/CO – Kennicutt, Regan, Murphy/Braun et al. • Systematic representative surveys (e.g. SINGS) – Separation of stars and different types of dust – Get full SED’s, star formation rates, resolved structures • Key challenge is to model all this in detail (Dopita)
0.15 µm 0.4-0.8 µm 1.2-2.2 µm 3.6 µm 8.0 µm 24 µm 70 µm 160 µm
Page 1 and 2: Nearly Normal Galaxies in a ΛCDM U
Page 3 and 4: Ascona/Terschelling Highlights •
Page 5 and 6: The outer regions of M31 Worthey, E
Page 11 and 12: NGC 4656: small bulge and prominent
Page 13 and 14: Ascona/Terschelling Highlights Disk
Page 15: Interpretations of disk truncations
Page 19 and 20: ΛCDM Formation Models • Failures
Page 21 and 22: ΛCDM Formation Models • predicti
Page 23 and 24: Effect of Adiabatic Contraction (sa
Page 25 and 26: Moving Forward in Mass Modeling Req
Page 29 and 30: An argument for pure stellar disks
Page 31 and 32: Residual Correlations Courteau et a
Page 33 and 34: Comparison With Models • Simple e
Page 36 and 37: Evidence for Sub-Maximal Disks •
Page 38 and 39: SparsePak Study of Barred Galaxies
Page 40 and 41: € Scaling Relations of Galaxies
Page 42 and 43: λ = halo spin c = halo conc. m d =

Stéphane Courteau

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