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The spectrum and dips of RE 0751+14: A joint evaluation of ROSAT and ASCA archival data

Kiziloglu, U
Baykal, Altan
Alev, M
Gogus, E
Using archival ASCA and ROSAT observations of RE 0751+14, X-ray energy spectra, pulse profiles and the results of pulse timing analysis are presented. The energy spectra are well-fitted by a blackbody model at low energy and a Raymond-Smith model at high energy, together with a partial covering absorber. A fluorescence emission line at 6.4 keV with an equivalent width similar to 220 eV was resolved for the first time.