Chemical abundances and spatial distribution of long gamma-ray bursts

We analyse the spatial distribution within host galaxies and chemical properties of the progenitors of long gamma-ray bursts (LGRBs) as a function of redshift. By using hydrodynamical cosmological simulations, which include star formation, supernova feedback and chemical enrichment, and based on the...

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Autores principales: Artale, M.C., Pellizza, L.J., Tissera, P.B.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00358711_v415_n4_p3417_Artale
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spelling todo:paper_00358711_v415_n4_p3417_Artale2023-10-03T14:47:00Z Chemical abundances and spatial distribution of long gamma-ray bursts Artale, M.C. Pellizza, L.J. Tissera, P.B. Galaxies: abundances Galaxies: evolution Gamma-ray burst: general We analyse the spatial distribution within host galaxies and chemical properties of the progenitors of long gamma-ray bursts (LGRBs) as a function of redshift. By using hydrodynamical cosmological simulations, which include star formation, supernova feedback and chemical enrichment, and based on the hypothesis of the collapsar model with low metallicity, we investigate the progenitors in the range 0 < z < 3. Our results suggest that the sites of these phenomena tend to be located in the central regions of the hosts at high redshifts but move outwards for lower ones. We find that scenarios with low metallicity cut-offs best fit current observations. For these scenarios, LGRBs tend to be [Fe/H]-poor and show a strong α-enhancement evolution towards lower values as redshift decreases. The variation of typical burst sites with redshift would imply that they might be tracing different parts of galaxies at different redshifts. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00358711_v415_n4_p3417_Artale
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Galaxies: abundances
Galaxies: evolution
Gamma-ray burst: general
spellingShingle Galaxies: abundances
Galaxies: evolution
Gamma-ray burst: general
Artale, M.C.
Pellizza, L.J.
Tissera, P.B.
Chemical abundances and spatial distribution of long gamma-ray bursts
topic_facet Galaxies: abundances
Galaxies: evolution
Gamma-ray burst: general
description We analyse the spatial distribution within host galaxies and chemical properties of the progenitors of long gamma-ray bursts (LGRBs) as a function of redshift. By using hydrodynamical cosmological simulations, which include star formation, supernova feedback and chemical enrichment, and based on the hypothesis of the collapsar model with low metallicity, we investigate the progenitors in the range 0 < z < 3. Our results suggest that the sites of these phenomena tend to be located in the central regions of the hosts at high redshifts but move outwards for lower ones. We find that scenarios with low metallicity cut-offs best fit current observations. For these scenarios, LGRBs tend to be [Fe/H]-poor and show a strong α-enhancement evolution towards lower values as redshift decreases. The variation of typical burst sites with redshift would imply that they might be tracing different parts of galaxies at different redshifts. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.
format JOUR
author Artale, M.C.
Pellizza, L.J.
Tissera, P.B.
author_facet Artale, M.C.
Pellizza, L.J.
Tissera, P.B.
author_sort Artale, M.C.
title Chemical abundances and spatial distribution of long gamma-ray bursts
title_short Chemical abundances and spatial distribution of long gamma-ray bursts
title_full Chemical abundances and spatial distribution of long gamma-ray bursts
title_fullStr Chemical abundances and spatial distribution of long gamma-ray bursts
title_full_unstemmed Chemical abundances and spatial distribution of long gamma-ray bursts
title_sort chemical abundances and spatial distribution of long gamma-ray bursts
url http://hdl.handle.net/20.500.12110/paper_00358711_v415_n4_p3417_Artale
work_keys_str_mv AT artalemc chemicalabundancesandspatialdistributionoflonggammaraybursts
AT pellizzalj chemicalabundancesandspatialdistributionoflonggammaraybursts
AT tisserapb chemicalabundancesandspatialdistributionoflonggammaraybursts
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