Abstract
GRB 170817A, associated with the LIGO-Virgo GW170817 neutron-star merger event, lacks the short duration and hard spectrum of a Short gamma-ray burst (GRB) expected from long-standing classification models. Correctly identifying the class to which this burst belongs requires comparison with other GRBs detected by the Fermi GBM. The aim of our analysis is to classify Fermi GRBs and to test whether or not GRB 170817A belongs—as suggested—to the Short GRB class. The Fermi GBM catalog provides a large database with many measured variables that can be used to explore gamma-ray burst classification. We use statistical techniques to look for clustering in a sample of 1298 gamma-ray bursts described by duration and spectral hardness. Classification of the detected bursts shows that GRB 170817A most likely belongs to the Intermediate, rather than the Short GRB class. We discuss this result in light of theoretical neutron-star merger models and existing GRB classification schemes. It appears that GRB classification schemes may not yet be linked to appropriate theoretical models, and that theoretical models may not yet adequately account for known GRB class properties. We conclude that GRB 170817A may not fit into a simple phenomenological classification scheme.
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Acknowledgements
We thank the support of the Fermi team, especially Drs. Bhat and Veres, for providing the hardness data. This research was supported by OTKA grant NN111016 and by NASA EPSCoR grant NNX13AD28A. Support for ÚNKP-17-3 New National Excellence Program of the Ministry of Human Capacities is appreciated (I.R.).
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Horváth, I., Tóth, B.G., Hakkila, J. et al. Classifying GRB 170817A/GW170817 in a Fermi duration–hardness plane. Astrophys Space Sci 363, 53 (2018). https://doi.org/10.1007/s10509-018-3274-5
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DOI: https://doi.org/10.1007/s10509-018-3274-5