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24 April 2024
 
  » arxiv » astro-ph/0211101

 Article overview



The XMM-Newton view of the radio-quiet neutron star 1E 1207.4-5209
A. De Luca ; S. Mereghetti ; P.A. Caraveo ; R.P. Mignani ; W. Becker ; G.F. Bignami ;
Date 6 Nov 2002
Subject astro-ph
Affiliation1,2), S. Mereghetti , P.A. Caraveo , R.P. Mignani , W. Becker and G.F. Bignami ( IASF/CNR sez. Milano, Milano, Italy; Universita’ di Milano Bicocca, Milano, Italy; ESO, Garching, Germany; MPE, Garching, Germany; Universita’ di Pavia,
AbstractWe have observed the radio-quiet X-ray pulsar 1E 1207.4-5209 with the high throughput EPIC cameras onboard XMM-Newton. The spectrum of this peculiar source is characterized by two broad absorption features which present significant substructures and show a clear phase-dependence. We believe that these features represent a strong evidence for the presence of a magnetized atmosphere containing heavy elements.
Source arXiv, astro-ph/0211101
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