High-resolution X-ray spectroscopy has become a powerful tool for
astrophysics since the launch of Chandra and XMM-Newton, ten years
ago. The grating spectrometers on both instruments still continue
to provide excellent data, while imaging calorimeters are being
prepared for future missions like Astro-H and IXO. The synergy with
other wavelength bands like the UV has been boosted by the addition
of COS to HST. X-ray spectroscopy offers unique diagnostics to
study almost any object in the Universe. This book contains review
papers on highlights and the state-of-the-art of X-ray spectroscopy
for a broad range of objects and on the prospects for future
studies.
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