INTEGRAL observation of the accreting pulsar GX 1+4

Abstract

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.

arXiv comment15 pages, 13 figures. Accepted for publication on Astronomy and Astrophysics. Introduced language editing corrections

References in corpus (22)

• ISGRI: the INTEGRAL Soft Gamma-Ray Imager
• Observations of Accreting Pulsars
• Statistics: Handle with Care, Detecting Multiple Model Components with the Likelihood Ratio Test
• Magnetic Fields of Accreting X-Ray Pulsars with the Rossi X-Ray Timing Explorer
• The INTEGRAL/IBIS Scientific Data Analysis
• Evidence for "Propeller" Effects In X-ray Pulsars GX 1+4 And GROJ1744-28
• The INTEGRAL IBIS/ISGRI System Point Spread Function and Source Location Accuracy
• On the Correlation of Torque and Luminosity in GX 1+4
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• First results from the INTEGRAL Galactic plane scans
• The Orbital Period of the Accreting Pulsar GX1+4
• INTEGRAL observations of the Crab pulsar
• Accretion column eclipses in the X-ray pulsars GX 1+4 and RX J0812.4-3114
• ASCA and Ginga Observations of GX 1+4
• A Compton reflection dominated spectrum in a peculiar accreting neutron star
• Detection of hard X-ray pulsations and a strong iron K_beta emission line during an extended low state of GX 1+4
• Cessation of X-ray Pulsation of GX 1+4
• Spectral variation in the X-ray pulsar GX 1+4 during a low-flux episode
• Accretion column disruption in GX 1+4
• Pulse Profiles, Accretion Column Dips and a Flare in GX 1+4 During a Faint State

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