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arXiv:astro-ph/0010642 (astro-ph)
[Submitted on 31 Oct 2000]

Title:Modelling the spin pulse profile of the isolated neutron star RX J0720.4--3125 observed with XMM-Newton

Authors:Mark Cropper (1), Silvia Zane (1), Gavin Ramsay (1), Frank Haberl (2)Christian Motch (3) ((1) MSSL, (2) MPE Garching, (3) Observatoire Astronomique, Strasbourg)
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Abstract: We model the spin pulse intensity and hardness ratio profiles of the isolated neutron star RXJ0720.4--3125 using XMM-Newton data. The observed variation is approximately sinusoidal with a peak-to-peak amplitude of 15%, and the hardness ratio is softest slightly before flux maximum. By using polar cap models we are able to derive maximum polar cap sizes and acceptable viewing geometries. The inferred sizes of the caps turn out to be more compatible with a scenario in which the neutron star is heated by accretion, and place limits on the magnetic field strength. The hardness ratio modulation can then be explained in terms of energy-dependent beaming effects, and this constrains the acceptable models of the emerging radiation to cases in which softer photons are more strongly beamed than harder photons. An alternative explanation in terms of spatially variable absorption co-rotating in the magnetosphere is also discussed.
Comments: accepted for publication in A&A special issue of XMM results, 6 pages
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0010642
  (or arXiv:astro-ph/0010642v1 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0010642
Related DOI: https://doi.org/10.1051/0004-6361%3A20000086

Submission history

From: Gavin Ramsay [view email]
[v1] Tue, 31 Oct 2000 13:57:44 UTC (31 KB)
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