Karl Glazebrook - Gemini Observatory

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Disk Galaxies at z~0 and z>1 z~0 86 z~2 Karl Glazebrook, SUT Friday, 3 August 12
z~0 Stellar thin disk σz ~ 20 km/s, hz~200–300 pc Stellar thick disk σz ~40 km/s, hz~1500 pc HI gas, molecular gas, GMCs, HII regions, OBA stars σz ~ 5 km/s, hz~50 pc (Note thermal 10 4 K broadening of Hα = 9 km/s) Karl Glazebrook, SUT Friday, 3 August 12
Page 1 and 2: Observations of local Turbulent Dis
Page 3 and 4: 1913LowOB...2...56S Sep 17 th 1912
Page 5: Origins of the Expanding Universe 1
Page 9 and 10: Galaxy morphologies at z>1 86 ELMEG
Page 11 and 12: sk c disk disk gas disk Unstable R
Page 13 and 14: uniformly in r, using the fact that
Page 15 and 16: High Hα SDSS galaxies? Star Format
Page 17 and 18: ) 1 d) .8 ° SDSS Three Colour Imag
Page 19 and 20: 2) Are they clumpy? Karl Glazebrook
Page 21 and 22: 2) Determining how early in the Uni
Page 23 and 24: Rob Bassett (Swinburne) 4) Are the
Page 25 and 26: Velocity Width HkmêsL Velocity Map
Page 27 and 28: Velocity Width HkmêsL Velocity Map
Page 29 and 30: Prediction: velocity dispersion of

Karl Glazebrook - Gemini Observatory

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