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Understanding the nature of the intriguing source X Persei: a deep look with a Suzaku observation
Stockholm University, Nordic Institute for Theoretical Physics (Nordita).
Number of Authors: 4
2017 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 470, no 1, 713-722 p.Article in journal (Refereed) Published
Abstract [en]

We present detailed broad-band timing and spectral analysis of the persistent, low luminosity and slowly spinning pulsar X Persei using a deep Suzaku observation of the source. The spectrum is unusually hard with a cyclotron resonance scattering feature (CRSF), the presence of which has been debated. By comparing the spectral models relevant for accretion-powered pulsars, we have obtained the best constraint on the broad-band spectral model of X Persei obtained so far. The CRSF is not confirmed in the average spectrum. We have also identified the presence of different intensity levels in the source with distinct changes in the pulse profile and the energy spectrum indicating changes in the accretion geometry. We further find evidence of a CRSF in the highest intensity levels at similar to 40 keV, indicating a magnetic field strength of 3.4 x 10(12) G.

Place, publisher, year, edition, pages
2017. Vol. 470, no 1, 713-722 p.
Keyword [en]
stars: neutron, X-rays: binaries, X-rays: individual: X Persei
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-147145DOI: 10.1093/mnras/stx1281ISI: 000406842600043OAI: oai:DiVA.org:su-147145DiVA: diva2:1144064
Available from: 2017-09-25 Created: 2017-09-25 Last updated: 2017-09-25Bibliographically approved

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Raichur, Harsha
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