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

Date

1998-01-01

Author

Kiziloglu, U
Baykal, Altan
Alev, M
Gogus, E

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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.

Subject Keywords

Intermediate polar Re-0751+14, X-Ray Observations, Magnetic-Field, Emission, Stars, Accretion, Am

URI

https://hdl.handle.net/11511/38740

Journal

ASTROPHYSICS AND SPACE SCIENCE

DOI

https://doi.org/10.1023/a:1001556513668

Collections

Department of Physics, Article

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Citation Formats

U. Kiziloglu, A. Baykal, M. Alev, and E. Gogus, “The spectrum and dips of RE 0751+14: A joint evaluation of ROSAT and ASCA archival data,” ASTROPHYSICS AND SPACE SCIENCE, pp. 191–203, 1998, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/38740.