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INTEGRAL observation of the accreting pulsar GX 1+4
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Ferrigno, C., Segreto, A., Santangelo, A., Wilms, J. (Joern), Kreykenbohm, I., Denis, M. (Mirosław) and Staubert, R.. (2007) INTEGRAL observation of the accreting pulsar GX 1+4. Astronomy & Astrophysics, Vol.462 (No.3). pp. 995-1005. ISSN 0004-6361
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Official URL: http://dx.doi.org/10.1051/0004-6361:20053878
Abstract
Aims. 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. Methods. The source was observed in different luminosity states ranging from L20−40 keV = 1.7 × 10−10 erg cm−2 s−1, to L20−40 keV = 10.5 × 10−10 erg cm−2 s−1 for about 779 ks from March 2003 until October 2004. Results. Our observations confirm the secular spin down of GX 1+4 with the spin period (Ps) 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 of 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 for an absorption feature at 34 ± 2 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 (2.9 ± 0.2) × 1012(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.
| Item Type: | Journal Article |
|---|---|
| Subjects: | Q Science > QB Astronomy |
| Divisions: | Faculty of Science > Physics |
| Library of Congress Subject Headings (LCSH): | Pulsars, X-ray sources, Galactic, Double stars |
| Journal or Publication Title: | Astronomy & Astrophysics |
| Publisher: | EDP Sciences |
| ISSN: | 0004-6361 |
| Date: | February 2007 |
| Volume: | Vol.462 |
| Number: | No.3 |
| Page Range: | pp. 995-1005 |
| Identification Number: | 10.1051/0004-6361:20053878 |
| Status: | Peer Reviewed |
| Access rights to Published version: | Open Access |
| Funder: | Agenzia spaziale italiana [Italian Space Agency] (ASI), Deutsche Forschungsanstalt für Luft- und Raumfahrt (DLR) |
| Grant number: | I/R/046/04 (ASI), ASI-INAF I/023/05/0 (ASI), 50 OG 9601 (DLR), 50 OG 0501 (DLR) |
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| URI: | http://wrap.warwick.ac.uk/id/eprint/3473 |
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