Other
Scientific paper
Sep 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001basi...29..355m&link_type=abstract
Bulletin of the Astronomical Society of India, Vol. 29, p. 355-360
Other
Scientific paper
Hard X-ray observations of the binary X-ray pulsars were made using a balloon-borne large area scintillation counter telescope in the 20-200 keV band. Apart from many other galactic and extragalactic X-ray sources, three X-ray pulsars namely Her X-1, GS 1843+00 and 4U 1907+09 were tracked during two flights launched in March 1997 and Nov. 1998. The observations of the transient sources GS 1843+00 correspond to near intensity maximum in its burst phase. We discuss the morphology of the pulse profiles in terms of geometrical constraints and the X-ray emission mechanism.
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