Polarization of Kilonova Emission from a Black Hole–Neutron Star Merger
Author:
Funder
National Nature Science Foundation of China
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab2387/pdf
Reference48 articles.
1. Type I supernovae. I - Analytic solutions for the early part of the light curve
2. SYSTEMATICS OF DYNAMICAL MASS EJECTION, NUCLEOSYNTHESIS, AND RADIOACTIVELY POWERED ELECTROMAGNETIC SIGNALS FROM NEUTRON-STAR MERGERS
3. Mergers of black hole–neutron star binaries and rates of associated electromagnetic counterparts
4. The origin of polarization in kilonovae and the case of the gravitational-wave counterpart AT 2017gfo
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1. Impact of jets on kilonova photometric and polarimetric emission from binary neutron star mergers;Monthly Notices of the Royal Astronomical Society;2023-05-25
2. Light Curves and Polarizations of Gravitationally Lensed Kilonovae;The Astrophysical Journal;2023-02-01
3. Coalescence of black hole–neutron star binaries;Living Reviews in Relativity;2021-12
4. Polarized kilonovae from black hole–neutron star mergers;Monthly Notices of the Royal Astronomical Society;2020-12-10
5. Kilonova Emission from Black Hole–Neutron Star Mergers. I. Viewing-angle-dependent Lightcurves;The Astrophysical Journal;2020-06-29
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