High-energy Phenomena in the Universe from Recent Chandra and XMM-Newton Observations

Details High-energy Phenomena in the Universe from Recent Chandra and XMM-Newton Observations High-energy Phenomena in the Universe from Recent Chandra and XMM-Newton Observations

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apr.t1001s&link_type=abstract

American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #T1.001

Physics

Scientific paper

The advent of the Chandra and XMM-Newton X-ray Observatories, with complementary capabilities, has opened a new window to study high-energy emission from extragalactic sources. Thanks to the unprecedented angular resolution provided by Chandra and the high throughput afforded by XMM-Newton, detailed imaging spectroscopy of relatively faint X-ray sources is now possible. In this talk, I will review recent discoveries from the two Observatories, with particular emphasis on the study of black holes in galaxies, and related phenomena.

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