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Supernova kicks and misaligned Be star binaries

✍ Scribed by Rebecca G. Martin; Christopher A. Tout; J. E. Pringle


Book ID
110847731
Publisher
John Wiley and Sons
Year
2009
Tongue
English
Weight
947 KB
Volume
397
Category
Article
ISSN
0035-8711

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The spin periods of accreting neutron stars in binary systems with Be star primaries are shown to depend more strongly on periastron distance than apastron distance. This is interpreted as showing that neutron stars spin-up on shorter timescales than they spin-down. The pulse and orbital periods of