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

We propose a new formation channel for intermediate mass black hole (IMBH)binaries via globular cluster collisions in the Galactic disc. Using numericalsimulations, we show that the IMBHs form a tight binary that enters thegravitational waves (GWs) emission dominated regime driven by stellarinteractions, and ultimately merge in $\lesssim 0.5$ Gyr. These events areclearly audible to LISA and can be associated with electromagnetic emissionduring the last evolutionary stages. During their orbital evolution, the IMBHsproduce runaway stars comparable with GAIA and LAMOST observations.

Mergers of globular clusters in the Galactic disc: intermediate mass black hole coalescence and implications for gravitational waves detection