Balloon Observations of High Energy X-ray Sources in the Region of the Galactic Centre

Details Balloon Observations of High Energy X-ray Sources in the Region of the Galactic Centre Balloon Observations of High Energy X-ray Sources in the Region of the Galactic Centre

Sep 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.223.1142l&link_type=abstract

Nature, Volume 223, Issue 5211, pp. 1142-1143 (1969).

Physics

11

Scientific paper

IN an eight-hour balloon flight launched from Mildura, Australia, on October 15, 1967, we surveyed the X-ray emission above 20 keV from the region of the sky from declinations -70° to -5° and from right ascensions 150° to 280° (angular resolution 13° f.w.h.m.). We noted earlier1 that the data showed several sources in a region near the galactic centre. From a more detailed analysis of the data from this region we can now account for the bulk of the hard X-rays we observed in terms of four sources whose positions and spectra we report here.

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