Search for pre-burst emission from binary neutron star mergers with 
Spectrum-Roentgen-Gamma

Mereminskiy, I. A.; Lutovinov, A. A.; Postnov, K. A.; Arefiev, V. A.; Lapshov, I. Yu.; Molkov, S. V.; Sazonov, S. Yu.; Semena, A. N.; Tkachenko, A. Yu.; Shtykovsky, A. E.; Liu, Z.; Wilms, J.; Rau, A.; Kreykenbohm, T. Dauser & I.

doi:10.1134/S1063773722070064

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Search for pre-burst emission from binary neutron star mergers with Spectrum-Roentgen-Gamma

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Liu, Z.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Rau, A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Mereminskiy, I. A., Lutovinov, A. A., Postnov, K. A., Arefiev, V. A., Lapshov, I. Y., Molkov, S. V., et al. (2022). Search for pre-burst emission from binary neutron star mergers with Spectrum-Roentgen-Gamma. Astronomy Letters-a Journal of Astronomy and Space Astrophysics, 48(7), 370-375. doi:10.1134/S1063773722070064.

Cite as: https://hdl.handle.net/21.11116/0000-000C-9F82-E

Abstract

Close binary systems consisting of two neutron stars (BNS) emit gravitational waves, that allow them to merge on timescales shorter than Hubble time. It is widely believed, that NS–NS mergers in such systems power short gamma-ray bursts (GRB). Several mechanisms which could lead to electromagnetic energy release prior to a merger have been proposed. We estimate the ability to observe the possible pre-burst emission with telescopes of Spectrum–Roentgen–Gamma. We also investigate first such event, GRB210919A, which fell into the field of view of the SRG telescopes less than two days before the burst.