ISSN:
1476-4687
Source:
Nature Archives 1869 - 2009
Topics:
Biology
,
Chemistry and Pharmacology
,
Medicine
,
Natural Sciences in General
,
Physics
Notes:
[Auszug] If the 0.5-ms pulses are due to rotation, then bounds on the supernova-remnant energy excess imply a polar field strength B=^109 G (ref. 1). If, however, the pulses are due to radial oscillations excited at the neutron star's birth, then the require-ment that rotation-dependent gravitational ...
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1038/340699a0
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