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in order to reconcile CDM with galaxy observations, there must be a strongly non ... cold gas (and metals) heated and ejected from the galaxy ...
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Most of the action is in the big cities. Newcomers to the city are rapidly stripped of (almost! ... Sizes of disks and bulges. Observed distribution ~ Lognormal ...
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Star Formation Downsizing: Testing the Role of Mergers and AGN
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Large-scale homogeneity & isotropy. 3. Primordial nucleosynthesis. 4. CMB. ... Polarization measurements can substantially improve accuracy with which ...
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SemiAnalytic Galaxy Formation are we kidding ourselves
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New Results from the Cosmic Background Imager
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National Radio Astronomy Observatory. Socorro, NM. Patricia Udomprasert, and the CBI Team ... Discovered 1965 (Penzias & Wilson) 2.7 K blackbody. Isotropic ...
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(2 billion light yrs) INNER RING (6 billion light yrs) OUTER RING (11 billion light yrs) ... Dark matter halo! (Atoms) Really? Is there dark matter? Cosmic ...
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Two sets: L = 25 Mpc/h to z=2. L = 100 Mpc/h to z=0 ... Many groups use (nearly) the same subgrid recipes. Insufficient awareness of models ingredients ...
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the faint end of the luminosity function of galaxies depends on environment ... galaxy appears to be a normal dIrr, with HI and leisurely ongoing star formation. ...
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Digging for new (Astro-)Physics in the old CMB. Niayesh Afshordi ... Digging for new (Astro-)Physics in the old CMB. 2. Outline. 1-Tracing dark forces on large scales ...
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Inflation, Gravity Waves and the CMB
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21 cm radio emission as a probe of Reionization. Cross-Correlation of ... Moving Halo Effect (Birkinshaw & Gull 1983) Thermal Sunyaev-Zel'dovich (SZ) Effect ...
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Cosmology from Gravity, Galaxies and Gas
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LAB survey. Bruns et al. 05. Braun & Thilker 04 ... Latest observational (HI) results: ... If in free expansion, mean expansion time 10 Myr, very short. ...
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