Ariel 5 hard X-ray observations

Details Ariel 5 hard X-ray observations Ariel 5 hard X-ray observations

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979rspsa.366..295q&link_type=abstract

(Royal Society, Discussion on Some Recent Results in X-Ray Astronomy, London, England, Apr. 25, 26, 1978.) Royal Society (London

Astronomy and Astrophysics

Astronomy

Ariel 5 Satellite, Binary Stars, Pulsars, Stellar Winds, X Ray Sources, Bursts, Graphs (Charts), Mass Transfer, Periodic Variations, White Dwarf Stars, X Ray Spectra

Scientific paper

Results obtained with the hard X-ray detector aboard Ariel 5 are reviewed. Various theoretical expectations for the form of X-ray source spectra are discussed. Results are examined for specific binary pulsars, sources with aperiodic fluctuations and power-law spectra, Sco X-1 type objects, white-dwarf X-ray emitters, COS-B sources, and X-ray bursters. The objects are classified according to the probable X-ray emission mechanism near the X-ray star or on the basis of the presence of a stellar wind or the mass-transfer mechanism involving Roche-lobe overflow.

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