Capabilities of spectroscopy in the context of X-ray astronomy in the 1900's

Details Capabilities of spectroscopy in the context of X-ray astronomy in the 1900's Capabilities of spectroscopy in the context of X-ray astronomy in the 1900's

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.239....5c&link_type=abstract

In ESA Proceedings of ESA Workshop on a Cosmic X-Ray Spectroscopy Mission p 5-14 (SEE N86-22461 12-89)

Astronomy and Astrophysics

Astronomy

European Space Programs, Nasa Programs, Spaceborne Astronomy, X Ray Astronomy, X Ray Spectroscopy, Galaxies, Interstellar Space, Spaceborne Telescopes, Stars, Supernova Remnants, Surveys, X Ray Telescopes

Scientific paper

The mission philosophies and parameters of the NASA AXAF and ESA XMM X-ray astronomy observatories are reviewed. The scientific topics that require an observatory of the XMM class are outlined and the relevance of angular and spectral resolution to these aims is discussed. The observing requirements of surveys and point source detection; galatic clusters; active galatic nuclei; normal galaxies and halos; stars; X-ray binaries; supernova remnants; and the interstellar medium are considered.

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