Using XMM-Newton to measure the spectrum of the Vela pulsar and its phase variation

  • Armando Manzali
  • Andrea De Luca
  • Patrizia A. Caraveo
Conference paper


We report on our analysis of two XMM-Newton observations of the Vela pulsar performed in December 2000 (total exposure time: 96.5 ks). We succeeded in resolving the pulsar spectrum from the surrounding bright nebular emission taking advantage both of the accurate calibration of the EPIC point spread function and of the Chandra/HRC surface brightness map of the nebula. This made it possible to assess to pulsar spectral shape disentangling its thermal and non-thermal components. Exploiting the photon harvest, we have also been able to perform a phase-resolved study of the pulsar emission.


Pulsars: general Pulsars: individual (Vela) Stars: neutron X-rays: stars 


97.60.Gb 97.60.Jd 98.70.Qy 


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Copyright information

© Springer 2007

Authors and Affiliations

  • Armando Manzali
    • 1
    • 2
  • Andrea De Luca
    • 1
  • Patrizia A. Caraveo
    • 1
  1. 1.INAF–IASFMilanoItaly
  2. 2.Dipartimento di Fisica Nucleare e TeoricaUniversità degli Studi di PaviaPaviaItaly

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