Needs and Requirements for Future X-Ray Observations of Hot Galactic Halos

Details Needs and Requirements for Future X-Ray Observations of Hot Galactic Halos Needs and Requirements for Future X-Ray Observations of Hot Galactic Halos

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000rmxac...9....6f&link_type=abstract

"Astrophysical Plasmas: Codes, Models, and Observations, Proceedings of the conference held in Mexico City, October 25-29, 1999,

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Galaxies are key objects for the study of cosmology, the life cycle of matter, and stellar evolution. X-ray observations have given us a new key window into these building blocks of the Universe, that allows us to investigate their hot gaseous component. While the study of these hot plasmas has important astrophysical and cosmological relevance, and significant advances in our knowledge are expected from Chandra and XMM, there are a number of fundamental questions that require a next generation of X-ray telescopes. These telescopes need to be 10-30 square-meter class telescopes, with Chandra-like resolution, and with a suite of instruments allowing spectral imaging at moderate to high resolution.

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