INTEGRAL observation of the accreting pulsar GX 1+4

Details INTEGRAL observation of the accreting pulsar GX 1+4 INTEGRAL observation of the accreting pulsar GX 1+4

2006-10-05

arxiv.org/abs/astro-ph/0610167v2

Astronomy and Astrophysics

Astrophysics

15 pages, 13 figures. Accepted for publication on Astronomy and Astrophysics. Introduced language editing corrections

Scientific paper

10.1051/0004-6361:20053878

We present the results of the INTEGRAL monitoring campaign on the accreting low mass X-ray binary pulsar GX 1+4 performed during the Galactic plane scan of the INTEGRAL Core Programme. The source was observed in different luminosity states ranging from L(20-40 keV)= 1.7x10^{-10} erg/cm^2/s, to L(20-40 keV)=10.5x10^{-10} erg/cm^2/s for about 779 ks from March 2003 until October 2004. Our observations confirm the secular spin down of GX 1+4 with the spin-period varying from 139.63 s to 141.56 s. In the highest luminosity state a spin-up phase is observed. The phase-averaged spectrum of the source was modelled either with an absorbed cut-off power law or with a Comptonization model with significantly different parameters in the two brightest luminosity states. No evidence for any absorption-like feature is observed in the phase-averaged spectrum up to 110 keV. At highest luminosity, the source is found to pulsate up to 130 keV. Phase-resolved spectroscopy reveals a phase-dependent continuum and marginal evidence of an absorption feature at 34 keV in the descending part of the pulse. If interpreted as due to electron resonant cyclotron scattering, the magnetic field in the emitting region would be 2.9x10^{12}(1+z) G where z is the gravitational red shift of the emitting region. We also observed a very low luminosity state typical of this source, which lasted for about two days during which the source spectrum was modelled by a simple power-law and a pulsed signal was still detectable in the 15-100 keV energy range.

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