Titlebook: Galaxies and their Masks; A Conference in Hono David L. Block,Kenneth C. Freeman,Ivanio Puerari Conference proceedings 2010 Springer Scienc

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Erdogan Madenci,Pranesh Roy,Deepak Beheragh this halo medium. Since the dwarfs are stripped at distances generally greater than 20 kpc, the gas is unlikely to make it directly into the spiral galaxy disk as cold star formation fuel. Some of the dwarfs’ gas may be integrated into the spiral galaxy’s hot halo and warm clumps may undergo a recooling process close to the disk.

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Lars Schweizer,Theodor Dingermannrived SN rates used for providing an independent measurement of the SF history of the Universe. We also present thus far the first NIR luminosity functions of super star cluster (SSC) candidates. The LFs can then be used to constrain the formation and evolution of SSCs via constraints based on initial mass functions and cluster disruption models.

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The Mask of Complexity in Disk Galaxies, of galaxies; only with such a complexity reduction we can claim to understand what are galaxies. Thus complexity acts as a mask which can be sometimes removed, unveiling the hidden simplicity of galaxies.