๐”– Bobbio Scriptorium
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Single Be stars as binary ejecta?

โœ Scribed by S. A. Rinehart


Book ID
104465478
Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
200 KB
Volume
312
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