NASA NTRS · 19820031116
The 805 second X-ray pulsar H2252-035
Abstract
It is shown that the X-ray flux from the 3.6 hr binary system H2252-035 is modulated at a period of 805 sec, and that its spectrum is consistent with either (1) a 1.4 photon index power law, or (2) a greater-than-20-keV thermal model. A 560 + or - 350 eV equivalent-width iron line at about 6.7 keV is noted, and the possibility that the H2252-035 system contains a slowly rotating neutron star is discussed.
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White, N. E., Marshall, F. E.. 1981-10-01. The 805 second X-ray pulsar H2252-035. https://ntrs.nasa.gov/citations/19820031116
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