{
  "id": "1507.00595",
  "version": "v1",
  "published": "2015-07-02T14:17:27.000Z",
  "updated": "2015-07-02T14:17:27.000Z",
  "title": "Luminosity-dependent spectral and timing properties of the accreting pulsar GX 304-1 measured with INTEGRAL",
  "authors": [
    "Christian Malacaria",
    "Dmitry Klochkov",
    "Andrea Santangelo",
    "Rüdiger Staubert"
  ],
  "comment": "12 pages, 12 figures, Accepted for publication in A&A",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Context: Be/X-ray binaries show outbursts with peak luminosities up to a few times $10^{37}\\,$erg/s, during which they can be observed and studied in detail. Most (if not all) Be/X-ray binaries harbour accreting pulsars, whose X-ray spectra in many cases contain cyclotron resonant scattering features related to the magnetic field of the sources. Spectral variations as a function of luminosity and of the rotational phase of the neutron star are observed in many accreting pulsars. Aims: We explore X-ray spectral and timing properties of the Be/X-ray binary GX 304-1 during an outburst episode. Specifically, we investigate the behavior of the cyclotron resonant scattering feature, the continuum spectral parameters, the pulse period, and the energy- and luminosity-resolved pulse profiles. We combine the luminosity-resolved spectral and timing analysis to probe the accretion geometry and the beaming patterns of the rotating neutron star. Methods: We analyze the INTEGRAL data from the two JEM-X modules, ISGRI and SPI, covering the January-February 2012 outburst, divided in six observations. We obtain pulse profiles in two energy bands, phase-averaged and phase-resolved spectra for each observation. Results: We confirm the positive luminosity-dependence of the cyclotron line energy in GX 304-1, and report a dependence of the photon index on luminosity. Using a pulse-phase connection technique, we find a pulse period solution valid for the entire outburst. Our pulse-phase resolved analysis shows, that the centroid energy of the cyclotron line is varying only slightly with pulse phase, while other spectral parameters show more pronounced variations. Our results are consistent with a scenario in which, as the pulsar rotates, we are exploring only a small portion of its beam pattern.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-07-02T14:17:27.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "accreting pulsar gx",
      "cyclotron resonant scattering feature",
      "timing properties",
      "luminosity-dependent spectral",
      "binaries harbour accreting pulsars"
    ],
    "publication": {
      "doi": "10.1051/0004-6361/201526417"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1380878
    }
  }
}