Pulsar timing in extreme mass ratio binaries: a general relativistic approach (2019)
Attributed to:
Dynamics of fast spinning neutron stars around a black hole
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stz845
Publication URI: http://dx.doi.org/10.1093/mnras/stz845
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1