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Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances

By Marco Palla and others
We identify the nature of high redshift long Gamma-Ray Bursts (LGRBs) host galaxies by comparing the observed abundance ratios in the interstellar medium with detailed chemical evolution models accounting for the presence of dust. We compare abundance data from long Gamma-Ray Bursts afterglow spectra to abundance patterns as predicted by... Show more
December 12, 2019
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Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
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