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 Plus annual

Presents the access of premium content as premium feature

Premium Content

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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The detection of gravitational waves emitted during a neutron star - blackhole merger and the associated electromagnetic counterpart will provide awealth of information about stellar evolution nuclear matter, and GeneralRelativity. While the theoretical framework about neutron star - black holebinaries formed in isolation is well established, the picture is looselyconstrained for those forming via dynamical interactions. Here, we use N-bodysimulations to show that mergers forming in globular and nuclear clusters coulddisplay distinctive marks compared to isolated mergers, namely larger masses,heavier black holes, and the tendency to have no associated electromagneticcounterpart. These features could represent a useful tool to interpretingforthcoming observations. In the Local Universe, gravitational waves emittedfrom dynamical mergers could be unravelled by detectors sensitive in thedecihertz frequency band, while those occurring at the distance range ofAndromeda and the Virgo Cluster could be accessible to lower-frequencydetectors like LISA.

Dissecting the properties of neutron star - black hole mergers originating in dense star clusters