EVIDENCE FOR A MASSIVE NEUTRON STAR FROM A RADIAL-VELOCITY STUDY OF THE COMPANION TO THE BLACK-WIDOW PULSAR PSR B1957+20
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/728/i=2/a=95/pdf
Reference53 articles.
1. Orbital period variability in the eclipsing pulsar binary PSR B1957+20: Evidence for a tidally powered star
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4. The masses of PSR J1911–5958A and its white dwarf companion
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