Constraining the star formation histories of GRB Host Galaxies from their observed abundance patterns

Abstract

Long-duration Gamma Ray Bursts (GRBs) are linked to the collapse of massive stars and their hosts are exclusively identified as active, star forming galaxies. Four long GRBs observed at high spectral resolution at redshift 1.5 <z < 4 allowed the determination of the elemental abundances for a set of different chemical elements. In this paper, for the first time, by means of detailed chemical evolution models taking into account also dust production, we attempt to constrain the star formation history of the host galaxies of these GRBs from the study of the chemical abundances measured in their ISM. We are also able to provide constraints on the age and on the dust content of GRB hosts. Our results support the hypothesis that long duration GRBs occur preferentially in low metallicity, star forming galaxies. We compare the specific star formation rate, namely the star formation rate per unit stellar mass, predicted for the hosts of these GRBs with observational values for GRB hosts distributed across a large redshift range. Our models predict a decrease of the specific star formation rate (SSFR) with redshift, consistent with the observed decrease of the comoving cosmic SFR density between z ~2 and z=0. On the other hand, observed GRB hosts seems to follow an opposite trend in the SSFR vs redshift plot, with an increase of the SSFR with decreasing redshift. Finally, we compare the SSFR of GRB050730 host with values derived for a sample of Quasar damped Lyman alpha systems. Our results indicate that the abundance pattern and the specific star formation rates of the host galaxies of these GRBs are basically compatible with the ones determined in Quasar damped Lyman alpha systems, suggesting similar chemical evolution paths.

15 pages, 11 figures, accepted by ApJ

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Cited by in corpus (11)

• A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium
• The dust-to-stellar mass ratio as a valuable tool to probe the evolution of local and distant star forming galaxies
• Modeling The GRB Host Galaxy Mass Distribution: Are GRBs Unbiased Tracers of Star Formation?
• A volume-limited sample of X-ray galaxy groups and clusters: III. Central abundance drops
• A new galactic chemical evolution model with dust: results for dwarf irregular galaxies and DLA systems
• Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
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• Chemical evolution models: GRB host identification and cosmic dust predictions
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• The nature of Long-GRB host galaxies from chemical abundances
• Self-consistent grain depletions and abundances I: The Orion Nebula as a test case