Neutron stars are the most poorly understood stellar objects in the Universe. But observations of X-rays emitted from one neutron star have now revealed a clue to the nature of its surface and composition.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on SpringerLink
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Miller, C. Nature 420, 31–33 (2002).
Bignami, G. F., Caraveo, P. A., De Luca, A., & Mereghetti, S. Nature 423, 725–727 (2003).
Zavlin, V. E. & Pavlov, G. G. in Proc 270. WE-Heraeus Seminar on Neutron Stars, Pulsars, and Supernova Remnants (eds Becker, W., Lesch, H. & Trümper, J.) 263–272 (Max Planck Inst. Extraterrestr. Phys., Garching, 2002).
Sanwal, D., Pavlov, G. G., Zavlin, V. E. & Teter, M. A. Astrophys. J. 574, L61–L64 (2002).
Hailey, C. J. & Mori, K. Astrophys. J. 578, L133–L136 (2002).
Mori, K. & Hailey, C. J. Preprint astro-ph/0301161 at <http://arXiv.org> (2003).
Trümper, J. et al. Astrophys. J. 219, L105–L110 (1978).
Haberl, F., Schwope, A. D., Hambaryan, V., Hasinger, G. & Motch, C. Astron. Astrophys. 403, L19–L23 (2003).
Duncan, R. C. & Thompson, C. Astrophys. J. 392, L9–L13 (1992).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Paerels, F. Superficial resonance. Nature 423, 697–699 (2003). https://doi.org/10.1038/423697a
Issue Date:
DOI: https://doi.org/10.1038/423697a