X-Ray Wind Tomography of IGR J17252-3616

Details X-Ray Wind Tomography of IGR J17252-3616 X-Ray Wind Tomography of IGR J17252-3616

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..179m&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

X-Ray Binary Stars, Gamma-Rays, Astronomical Observations, Neutron Stars, X-Ray Binaries, Gamma-Ray, Observatories And Site Testing, Neutron Stars

Scientific paper

IGR J17252-3616, a highly absorbed High Mass X-ray Binary (HMXB) with Hydrogen column density NH~(2-4)×1023 cm-2, has been observed with XMM-Newton for about one month. Observations were scheduled in order to cover the orbital-phase space as much as possible. IGR J17252-3616 shows a varying column density NH and Fe Kα line when fit with simple phenomenological models. A refined orbital solution can be derived. Spectral timing analysis allows derivation of the wind properties of the massive star.

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