The X-ray pulsars 4U1145-61 and 1E1145.1-6141

Details The X-ray pulsars 4U1145-61 and 1E1145.1-6141 The X-ray pulsars 4U1145-61 and 1E1145.1-6141

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980stin...8017932w&link_type=abstract

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Pulsars, Stellar Spectra, X Ray Sources, Binary Stars, Line Spectra, Periodic Variations

Scientific paper

Observations of the X-ray sources near 4U1145-61 are presented. The presence of two periodicities at 291 and 297 seconds is confirmed. The location of the shorter period is isolated to within 3 arc minutes of 4U1145-61. The spectrum of 4U1145-61 is a power law out to at least 60 keV with a 500 eV EW iron line at 6.7 keV. The inferred spectrum of the other is absorbed. No evidence is found for a monotonic variation in either pulse period.

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