Science with the Constellation-X Observatory

Details Science with the Constellation-X Observatory Science with the Constellation-X Observatory

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999head....4.1719v&link_type=abstract

American Astronomical Society, HEAD meeting #4, #17.19; Bulletin of the American Astronomical Society, Vol. 31, p.720

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Constellation X-ray Mission is a high throughput X-ray facility emphasizing observations at high spectral resolution (E/Delta E ~ 300--3000), and broad energy bandpass (0.25--40 keV). Constellation-X will provide a factor of nearly 100 increase in sensitivity over current high resolution X-ray spectroscopy missions. It is the X-ray astronomy equivalent of large ground-based optical telescopes such as the Keck Observatory and the ESO Very Large Telescope. When observations commence toward the end of next decade, Constellation-X will address many fundamental astrophysics questions such as: the formation and evolution of clusters of galaxies; constraining the baryon content of the Universe; determining the spin and mass of supermassive black holes in AGN; and probing strong gravity in the vicinity of black holes.

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