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An Explanation for the Properties of the Millisecond X-ray Oscillations Detected in Neutron Stars in LMXBs and the Rarity of These Detections

Published in 2011 by Ka-Ho Lo, F. K. Lamb, S. Boutloukos, M. C. Miller ORCID
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

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