Neutron Star Mergers in Active Galactic Nucleus Accretion Disks: Cocoon and Ejecta Shock Breakouts
Document Type
Article
Publication Date
1-12-2021
Publication Title
Astrophysical Journal Letters
Volume
906
Issue
2
First page number:
1
Last page number:
7
Abstract
Neutron star mergers are believed to occur in accretion disks around supermassive black holes. Here we show that a putative jet launched from the merger of a binary neutron star (BNS) or a neutron star–black hole (NSBH) merger occurring at the migration trap in an active galactic nucleus (AGN) disk would be choked. The jet energy is deposited within the disk materials to power a hot cocoon. The cocoon is energetic enough to break out from the AGN disk and produce a bright X-ray shock breakout transient peaking at ~0.15 days after the merger. The peak luminosity is estimated as... (see full abstract in article).
Disciplines
Stars, Interstellar Medium and the Galaxy
Language
English
Repository Citation
Zhu, J.,
Zhang, B.,
Yu, Y.,
Gao, H.
(2021).
Neutron Star Mergers in Active Galactic Nucleus Accretion Disks: Cocoon and Ejecta Shock Breakouts.
Astrophysical Journal Letters, 906(2),
1-7.
http://dx.doi.org/10.3847/2041-8213/abd412