Geodetic Precession in Binary Neutron Stars
classification
🌌 astro-ph
keywords
binarygeodeticprecessionanalysisapplieddemonstrateddiscussedemission
read the original abstract
The most recent evidence for geodetic precession observed in binary radio pulsars is presented and discussed. It is demonstrated how an analysis of these results can be used to study theories of gravity, stellar evolution and pulsar emission theory. In order to highlight the observational strategies, an overview of the applied techniques is given.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.