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A long-period, violently variable X-ray source in a young supernova remnant

A De Luca1, P A Caraveo, S Mereghetti

  • 1Istituto Nazionale d'Astrofisica-Istituto di Astrofisica Spaziale e Fisica Cosmica, Via Bassini 15, I-20133 Milano, Italy. deluca@iasf-milano.inaf.it

Science (New York, N.Y.)
|July 11, 2006
PubMed
Summary

Observations reveal a slow, periodic X-ray source in the RCW 103 supernova remnant. This neutron star may be a peculiar magnetar, slowed by debris, challenging compact object evolution theories.

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