Using Long-term Millisecond Pulsar Timing to Obtain Physical Characteristics of the Bulge Globular Cluster Terzan 5
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/845/i=2/a=148/pdf
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1. Orbital period variability in the eclipsing pulsar binary PSR B1957+20: Evidence for a tidally powered star
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3. Star distribution around a massive black hole in a globular cluster
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