no code implementations • 29 Jan 2021 • S. Sett, R. P. Breton, C. J. Clark, M. H. Kerkwijk, D. L. Kaplan
We discuss potential explanations for the non-detection of a pulsar in the studied SNRs and conclude that sensitivity is still the most likely factor responsible for the lack of pulsars in some remnants.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
