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Kinematics of low-mass X-ray binaries and millisecond pulsars
Author(s) -
R. Ramachandran,
D. Bhattacharya
Publication year - 1997
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/288.3.565
Subject(s) - millisecond pulsar , physics , pulsar , millisecond , kinematics , astrophysics , low mass , monte carlo method , mass distribution , astronomy , stars , classical mechanics , statistics , mathematics , galaxy
The kinematic properties of low-mass X-ray binaries and millisecond pulsars have been studied with the help of a Monte Carlo simulation. It is found that the kinematic properties of these two populations are consistent with each other, which supports the idea that LMXBs are the progenitors of millisecond pulsars. The speed distribution of millisecond pulsars is seen to be quite different from that...

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