Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-06-30T13:08:59.896Z Has data issue: false hasContentIssue false
  • English
  • Français

PSR J0218+4232 in the energy band 1–10 keV observed with BeppoSAX

Published online by Cambridge University Press:  12 April 2016

Luciano Nicastro
Luciano Nicastro*
Affiliation:
Istituto di Fisica Cosmica con Applicazioni all’Informatica, CNR, Via U. La Malfa 153, I-90146 Palermo, Italy

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

On behalf of a large collaboration (see Mineo et al. (1999) for details) I present the results of a BSAX observation of PSR J0218+4232 which, for the first time, provides detailed information on the pulsar temporal and spectral emission properties in the broad energy band 1–10 keV.

Type
Part 5. High-Energy Observations
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 347 - 348
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Kuiper, L., Hermsen, W., Verbunt, F., Belloni, T. 1998, A&AS, 336, 545 Google Scholar
Mineo, T., Cusumano, G., Kuiper, L., et al. 2000, A&A, submittedGoogle Scholar
Navarro, J., de Bruyn, A.G., Frail, D.A., et al. 1995, ApJ, 455, L55 Google Scholar
Verbunt, F., Kuiper, L., Belloni, T., et al. 1996, A&A, 311, L9 Google Scholar