Skip to main content
SearchLoginLogin or Signup

Comparing Binary Pulsar Properties in the Field and in Globular Clusters

Presentation #110.75 in the session “Stellar/Compact (Poster)”.

Published onApr 01, 2022
Comparing Binary Pulsar Properties in the Field and in Globular Clusters

We review the properties of observed populations of radio pulsars in the Milky Way field and globular clusters, contrasting in particular binary properties and taking into account selection effects. Using a combination of Monte Carlo dynamical modeling for dense star clusters and population synthesis for the field, we discuss how the observations compare to theoretical expectations from binary evolution and stellar dynamics.


Comments
0
comment

No comments here