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The possible companions of young radio pulsars

โœ Scribed by Simon F. Portegies Zwart; Lev R. Yungelson


Publisher
John Wiley and Sons
Year
1999
Tongue
English
Weight
131 KB
Volume
309
Category
Article
ISSN
0035-8711

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Stars usually form as members of binary or multiple star systems, and it is likely that the Sun was no exception. The mass and position of possible past companions of the Sun is determined by considering the orbital stability of the Solar System. This is achieved by considering the stability of crit