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Page 1: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 2: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 3: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 4: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 6: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 7: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 8: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 9: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 10: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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Page 11: Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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7/21/2019 Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

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