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GRB 190919B: Rapid optical rise explained as a flaring activity

By Martin Jelínek and others at
LogoASTRON
and
LogoMasaryk University
Following the detection of a long GRB 190919B by INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory), we obtained an optical photometric sequence of its optical counterpart. The light curve of the optical emission exhibits an unusually steep rise ~100 s after the initial trigger. This behaviour is not expected from a 'canonical'... Show more
March 21, 2022
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GRB 190919B: Rapid optical rise explained as a flaring activity
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