Resolving the Hard X-ray Emission of GX 5-1 with INTEGRAL

Details Resolving the Hard X-ray Emission of GX 5-1 with INTEGRAL Resolving the Hard X-ray Emission of GX 5-1 with INTEGRAL

2005-07-15

arxiv.org/abs/astro-ph/0507378v1

Astronomy and Astrophysics

Astrophysics

10 pages, 17 figures, accepted for publication in A&A

Scientific paper

10.1051/0004-6361:20041647

We present the study of one year of INTEGRAL data on the neutron star low mass X-ray binary GX 5-1. Thanks to the excellent angular resolution and sensitivity of INTEGRAL, we are able to obtain a high quality spectrum of GX 5-1 from ~5 keV to ~100 keV, for the first time without contamination from the nearby black hole candidate GRS 1758-258 above 20 keV. During our observations, GX 5-1 is mostly found in the horizontal and normal branch of its hardness intensity diagram. A clear hard X-ray emission is observed above ~30 keV which exceeds the exponential cut-off spectrum expected from lower energies. This spectral flattening may have the same origin of the hard components observed in other Z sources as it shares the property of being characteristic to the horizontal branch. The hard excess is explained by introducing Compton up-scattering of soft photons from the neutron star surface due to a thin hot plasma expected in the boundary layer. The spectral changes of GX 5-1 downward along the "Z" pattern in the hardness intensity diagram can be well described in terms of monotonical decrease of the neutron star surface temperature. This may be a consequence of the gradual expansion of the boundary layer as the mass accretion rate increases.

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