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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Near-IR Spectroscopy and Population Synthesis of Super Star Clusters in NGC 1569ry. We fit these photospheric spectra to NextGen model atmospheres to obtain effective spectral types of clusters, and find that the information in both .- ..-band spectra is necessary to remove degeneracy in the fits. The light of SSC B is unambiguously dominated by K0 supergiants (T. = 4400 ± 100

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Starbursts Near and Far: An Overvieww high effective temperatures; 4.) determination of the initial mass function in starbursts; 5.) the nature of LINERs; and 6.) whether the huge masses deduced for the ISM in starburst regions are correct.

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Star Formation in the Galactic Center and Nearby Nucleintly been born into massive stellar clusters. I discuss these findings and argue that the same considerations apply to most, if not all gas-rich spiral galaxies. In the mass budget of the Galactic center, star formation is apparently the dominant sink.

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Spectroscopy of Compact Star Clusters in NGC 4038/4039small spatial scales are seen throughout the merger. Cluster masses range from 10. to a few x 10. M.. A comparison between dynamically determined masses and those estimated from photometry in combination with starburst models suggests variations in the IMF from cluster to cluster.

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