English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

Exploiting a five-year span of data, we present improved timing solutions forthe five millisecond pulsars known in the globular cluster NGC 6752. Theyinclude proper motion determinations for the two outermost pulsars in thecluster, PSR J1910-5959A and PSR J1910-5959C. The values of the proper motionsare in agreement with each other within current uncertainties, but do not match(at 4 sigma and 2 sigma level respectively) with the value of the proper motionof the entire globular cluster derived in the optical band. Implications ofthese results for the cluster membership of the two pulsars are investigated.Prospects for the detection of the Shapiro delay in the binary systemJ1910-5959A are also discussed.Comment: 8 pages, 3 figures, accepted for publication in Ap

Timing of Millisecond Pulsars in NGC 6752. II. Proper Motions of the Pulsars in the Cluster Outskirts