The high-throughput X-ray spectroscopy mission: The mission-science report

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Spectroscopy, Esa Satellites, European Space Programs, Spaceborne Astronomy, X Ray Astronomy, X Ray Spectroscopy, Interstellar Space, Stellar Atmospheres, Stellar Radiation, Supernova Remnants

Scientific paper

The high throughput X-ray spectroscopy mission (XMM) of ESA and the astrophysics problems it addresses are described. The spaceborne XMM observatory offers spatial resolution within 30 arcsec (half energy width); effective area 6000 sq cm at 2 keV and 300 sq cm at 7 keV; Broadband (0.1 to 10 keV) spectroscopy with a resolving power (FWHM) between 5 and 60; medium-resolution spectroscopy between 0.1 to 3 keV with a resolving power of over 250 at 0.5 keV; and simultaneous optical monitoring between 2000 and 6000 A to a limiting magnitude of 24.5. Topics studied include large/medium scale structure of hot matter in the Universe; accretion-powered radiation sources; supernova remnants; the interstellar medium; and stellar atmospheres.

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