Orbital Phase Resolved Spectroscopy of EX Hya Using XMM-NEWTON

We present for the first orbital phase resolved spectra of intermediate polar (IP), EX Hya, during two different states with a factor of 3 difference between the X-ray count rates. We find definite spectral variations between different states of the source. The adopted model is composed of two MEKAL...

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Veröffentlicht in:	Proceedings of the International Conference 2009-09, Vol.1248, p.137-138
Hauptverfasser:	Pekon, Yakup, Balman, Solen
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption Accretion disks Continuums Counting Emission Gaussian IP (Internet Protocol) Mathematical models Orbitals Reflection Spectra Spectroscopy X-rays XMM (spacecraft)
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