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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0930-8989 d star formation are often located towards the centers of host galaxies. Studies of this kind of star formation at high redshift have produced astonishing results over recent years that were only possible with the latest generation of large ground-based and space telescopes. The papers collected in

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The Initial Mass Function in the Galactic Centerheoretical grounds. I will discuss these recent results, along with evidence for star formation in the immediate vicinity of the super massive black hole at the Galactic Center. The results of this work might be useful in extrapolating to other galactic centers with similar conditions, as well as other starburst regions.

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Nearby Dusty Starbursts and have extremely high star forming efficiency. Further advances will require improvements in the way boundary conditions such as bolometric and K-band luminosity, ionizing star effective temperature, and supernova rate are estimated and applied in the models.

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Evidence in Favour of IMF Variationse empirical evidence that the IMF varies with time, with environment, and for all stellar masses. While I see no obvious systematic trend in most regions of our Galaxy, there is at least an indication that the IMF is biased towards more massive stars in the early universe and in starbursts.

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0930-8989 this volume present these results in the context of the much firmer foundation of star formation in the local universe, and they emphasize all the important topics, from star formation in different environments to the cosmic star formation history.978-3-642-62562-6978-3-642-56538-0Series ISSN 0930-8989 Series E-ISSN 1867-4941

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The Initial Mass Function in the Galactic Center results suggest that the Galactic Center environment produces massive clusters with relatively flat initial mass functions, as might be expected on theoretical grounds. I will discuss these recent results, along with evidence for star formation in the immediate vicinity of the super massive black h