Concluding Reflections, Absorptions, and Scatterings

Details Concluding Reflections, Absorptions, and Scatterings Concluding Reflections, Absorptions, and Scatterings

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..761..451g&link_type=abstract

THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP Conference Pr

Physics

Magnitudes And Colors, Luminosities

Scientific paper

Multi-wavelength observations of the spectral energy distributions of galaxies now routinely cover from the X-rays to radio for systems ranging over more than 10 Gyr in lookback times. The interpretation of these data rests on understanding how galaxies produce and radiate their photon luminosities. This workshop provided a forum for discussion of our current understanding of this topic with an emphasis on how radiation supplied by local sources, stars or AGN, is transferred and reprocessed as it traverses the dusty ISM of galaxies. These concluding remarks discuss several of the main topics of the meeting along with outstanding issues and possibilities for future work.

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