DOAJ Open Access 2026

The Maximum Offsets of Binary Neutron Star Mergers from Host Galaxies

Ilya Mandel Om Sharan Salafia Andrew Levan Paul Disberg

Abstrak

We analytically derive, and illustrate with a population synthesis model, the maximum offset of binary neutron star mergers ejected from their host galaxies. This approximate maximum offset is 300 kpc $\times \,{({v}_{{\rm{esc}}}/500\,{\rm{km}}\,{{\rm{s}}}^{-1})}^{-7}$ , where v _esc is the escape velocity from the host galaxy. Massive hosts with high escape velocities are unlikely to yield very large offsets. This maximum offset should inform the host associations of mergers that are not coincident with galaxies. We also discuss potential correlations between offsets and system masses, and possibly the duration of the gamma-ray burst accompanying the merger.

Topik & Kata Kunci

Penulis (4)

I

Ilya Mandel

O

Om Sharan Salafia

A

Andrew Levan

P

Paul Disberg

Format Sitasi

Mandel, I., Salafia, O.S., Levan, A., Disberg, P. (2026). The Maximum Offsets of Binary Neutron Star Mergers from Host Galaxies. https://doi.org/10.3847/2041-8213/ae4332

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Informasi Jurnal
Tahun Terbit
2026
Sumber Database
DOAJ
DOI
10.3847/2041-8213/ae4332
Akses
Open Access ✓