Electromagnetic Counterparts of Binary-neutron-star Mergers Leading to a Strongly Magnetized Long-lived Remnant Neutron Star

We explore the electromagnetic counterparts that will associate with binary-neutron-star mergers for the case that remnant massive neutron stars survive for ≳0.5 s after the merger. For this study, we employ the outflow profiles obtained by long-term general-relativistic neutrino-radiation magnetohy...

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Veröffentlicht in:	The Astrophysical journal 2022-07, Vol.933 (1), p.22
Hauptverfasser:	Kawaguchi, Kyohei, Fujibayashi, Sho, Hotokezaka, Kenta, Shibata, Masaru, Wanajo, Shinya
Format:	Artikel
Sprache:	eng
Schlagworte:	Afterglows Amplification Astrophysics Binary stars Black holes Gravitational wave astronomy Infrared emissions Luminosity Magnetic fields Magnetohydrodynamic simulation Magnetohydrodynamics Near infrared radiation Neutrinos Neutron stars Neutrons Radiation Radiative transfer Radiative transfer simulations Star mergers Stars & galaxies Stellar magnetic fields Synchrotrons
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