Titlebook: New Extragalactic Perspectives in the New South Africa; Proceedings of the I David L. Block,J. Mayo Greenberg Conference proceedings 1996 K

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Optical, IR, and HI Observations of a Large Complete Cluster Sampleecified selection criteria within the volume of the cluster can be included. For example, a flux threshold might be set in some spectral band and this threshold corresponds to a specific . threshold for a complete sample.

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Organics and Ices in Galactic Dust. Laboratory organics produced by different processes are compared to the DISM features. The 3.4 .m feature has now been detected in other galaxies, which suggests that the widespread distribution of organic material in our own galaxy may be common to other galaxies as well.

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Temperature Fluctuations and Very Cold Dust the average temperature between high temperature spikes and will spend the majority of the time at these low temperatures. As a result, they will contribute excess emission at very . infrared wavelengths and this emission will be seen in IRAS sources at . wavelengths.

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The Effects of Supergiants on the Infrared Light Distribution in Galaxiesue to giant stars, ～ 7% due to main sequence stars, and only ～ 1% due to supergiants. Since main sequence stars, which dominate the mass, and giants are well–mixed in older populations (see Aaronson 1977 and Frogel 1988), K images should trace the mass effectively.

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