Please use this identifier to cite or link to this item: https://scidar.kg.ac.rs/handle/123456789/9607
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dc.rights.licenseopenAccess-
dc.contributor.authorSimić, Saša-
dc.contributor.authorPopović L.-
dc.date.accessioned2020-09-19T18:41:40Z-
dc.date.available2020-09-19T18:41:40Z-
dc.date.issued2012-
dc.identifier.issn0218-2718-
dc.identifier.urihttps://scidar.kg.ac.rs/handle/123456789/9607-
dc.description.abstractUsing the modified internal shock wave model, we fit the gamma ray burst (GRB) light and spectral curves of 30 GRBs observed with BATSE. From the best fitting, we obtain basic parameters of the relativistic shells which are in good agreement with predictions given earlier. We compare measured GRB parameters with those obtained from the model and discuss connections between them in the frame of the physical processes laying behind GRB events. © 2012 World Scientific Publishing Company.-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.sourceInternational Journal of Modern Physics D-
dc.titlePhysical parameters of the relativistic shock waves in GRBs: The case of 30 GRBs-
dc.typearticle-
dc.identifier.doi10.1142/S0218271812500289-
dc.identifier.scopus2-s2.0-84859736952-
Appears in Collections:Faculty of Science, Kragujevac

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