May 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pnas...96.5351k&link_type=abstract
Proceedings of the National Academy of Sciences of the United States of America, Volume 96, Issue 10, pp. 5351-5352
Physics
21
Scientific paper
Recent x-ray observations have shown that a substantial fraction of
newly born neutron stars have magnetic fields of several 1014
G. They reveal themselves as soft gamma repeaters and anomalous x-ray
pulsars and may account for the missing radio pulsars in young supernova
remnants.
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