Computer Science – Sound
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.170..569t&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 170, Mar. 1975, p. 569-577. Research supported by the Rothmans Universi
Computer Science
Sound
4
Balloon Sounding, Galactic Nuclei, Galactic Radiation, Radiant Flux Density, Spaceborne Astronomy, X Ray Sources, Galactic Structure, Milky Way Galaxy, Satellite Observation, Uhuru Satellite, X Ray Stars
Scientific paper
A reanalysis of University of Adelaide balloon data supports the conclusion that the dominant hard X-ray source in the Galactic center is GX1 + 4. Data are also presented for GX354-5. The hard source Ara XR-1 is probably the Uhuru object 3U 1705-44 and is variable by a factor of at least 1.7 times (20-40 keV). Nor XR-1 is difficult to identify and in common with the rocket object Nor X-1, no convincing Uhuru candidate exists. Ambiguities in pre-Uhuru nomenclature are pointed out with regard to these sources.
Buselli G.
Clancy M. C.
Davison J. N. P.
Thomas Rajat M.
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