Abstract
The nature of Gamma-Ray Burst (GRB) has been the object of many investigations but their origin has remained a mistery primarily for the difficulties in finding a counterpart. This difficulty derived from the intrinsically poor positioning capability of available GRB detectors.
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Piro, L. (1998). Discovery of X-Ray Counterparts to Gamma Ray Bursts by Bepposax. In: Koyama, K., Kitamoto, S., Itoh, M. (eds) The Hot Universe. International Astronomical Union / Union Astronomique Internationale, vol 188. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4970-9_38
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DOI: https://doi.org/10.1007/978-94-011-4970-9_38
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-5059-0
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