X-ray astronomy in the future

Details X-ray astronomy in the future X-ray astronomy in the future

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...30..537c&link_type=abstract

(European Space Agency, ESLAB Symposium on X-ray Astronomy, 15th, Amsterdam, Netherlands, June 22-26, 1981.) Space Science Revie

Mathematics

Logic

2

Satellite Observation, Spaceborne Astronomy, Technological Forecasting, X Ray Astronomy, X Ray Astrophysics Facility, X Ray Sources, Astronomical Maps, Astronomical Photography, Classifications, Sky Surveys (Astronomy), X Ray Telescopes

Scientific paper

It is shown how, from a beginning in 1962, X-ray observations have reached a position of prime importance in astronomy. It is thought that, in the 1980s, significant progress will come in two areas. One is the physics of bright X-ray sources, the other is sky surveys and the study of all detectable sources. For purposes of classification, bright sources are taken as those giving rise to fluxes greater than 1 microJy.

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