Titlebook: Starburst Galaxies: Near and Far; Proceedings of a Wor Linda Tacconi,Dieter Lutz Conference proceedings 20011st edition Springer-Verlag Ber

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Evidence Supporting the Universality of the IMFg photons in a population of some age and metallicity, through the creation rate of various chemical elements, to the mass to light ratio of a system. This significance, together with the empirical difficulty to determine the IMF robustly, and the near complete lack of any robust theoretical predict

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Star Formation in the Galactic Center and Nearby Nucleixy, despite the very different physical conditions in the central environment: a strong dipole magnetic field, strong tidal forces, and a large internal velocity dispersion within the abundant molecular clouds. There are at least two pronounced differences in the properties of the stars that form ne

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Star Formation in Galactic Disksonal rate of 100–1000 M./year, there exists a much broader class of “normal” galaxies at z = 0 which do form stars at rates ranging from 0 (E+S0) to 10 M./year (BCDs), with the vast majority of normal disk galaxies doing it at 1 M./year. Much of what is known about the star formation properties of n

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Nearby Dusty Starburstsodeling developed around such techniques provides satisfactory fits to all the relevant observables. These models show that starbursts are short-lived and have extremely high star forming efficiency. Further advances will require improvements in the way boundary conditions such as bolometric and K-b

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Starbursts, Dark Matter and Dwarf Galaxy Evolutionir star formation is regulated. Both usually show evidence for stellar and gaseous disks. However, their total mass is dominated by dark matter. Gas rich dwarfs form with a range of disk structural properties. These have been arbitrarily separated into two classes on the basis of central surface bri

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