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dc.contributor.author
Piranomonte, S.
dc.contributor.author
Ward, P. A.
dc.contributor.author
Fiore, F.
dc.contributor.author
Vergani, S. D.
dc.contributor.author
D'Elia, V.
dc.contributor.author
Krongold, Y.
dc.contributor.author
Nicastro, F.
dc.contributor.author
Meurs, E. J. A.
dc.contributor.author
Chincarini, G.
dc.contributor.author
Covino, S.
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Della Valle, M.
dc.contributor.author
Fugazza, D.
dc.contributor.author
Norci, L.
dc.contributor.author
Sbordone, L.
dc.contributor.author
Stella, L.
dc.contributor.author
Tagliaferri, G.
dc.contributor.author
Burrows, D. N.
dc.contributor.author
Gehrels, N.
dc.contributor.author
Goldoni, P.
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Malesani, D.
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Mirabel Miquele, Igor Felix
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Pellizza González, Leonardo Javier
dc.contributor.author
Perna, R.
dc.date.available
2017-07-24T19:34:57Z
dc.date.issued
2008-12
dc.identifier.citation
Piranomonte, S.; Ward, P. A.; Fiore, F.; Vergani, S. D.; D'Elia, V.; et al.; Probing the complex environments of GRB host galaxies and intervening systems: high resolution spectroscopy of GRB050922C; EDP Sciences; Astronomy and Astrophysics; 492; 3; 12-2008; 775-785
dc.identifier.issn
0004-6361
dc.identifier.uri
http://hdl.handle.net/11336/21204
dc.description.abstract
Aims. The aim of this paper is to investigate the environment of gamma ray bursts (GRBs) and the interstellar matter of their host galaxies. Methods. To this purpose we use high resolution spectroscopic observations of the afterglow of RB050922C, obtained with UVES/VLT ∼ 3.5 h after the GRB event. Results. We found that, as for most high resolution spectra of GRBs, the spectrum of the afterglow of GRB050922C is complex. At least seven components contribute to the main absorption system at z = 2.1992. The detection of lines of neutral elements like MgI
and the detection of fine-structure levels of the ions FeII, SiII and CII allows us to separate components in the GRB ISM along the line of sight. Moreover, in addition to the main system, we analyzed the five intervening systems between z = 2.077 and z = 1.5664 identified along the GRB line of sight. Conclusions. GRB afterglow spectra are very complex, but full of information. This can be used to disentangle the contribution of the different parts of the GRB host galaxy and to study their properties. Our metallicity estimates agree with the scenario of GRBs exploding in low metallicity galaxies
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
EDP Sciences
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Gamma Rays: Bursts
dc.subject
Cosmology: Observations
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Galaxies: Abundances
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Galaxies: Ism
dc.subject.classification
Astronomía
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Ciencias Físicas
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
dc.title
Probing the complex environments of GRB host galaxies and intervening systems: high resolution spectroscopy of GRB050922C
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-07-18T17:17:28Z
dc.journal.volume
492
dc.journal.number
3
dc.journal.pagination
775-785
dc.journal.pais
Francia
dc.journal.ciudad
Les Ulis
dc.description.fil
Fil: Piranomonte, S.. Osservatorio Astronomico di Roma; Italia
dc.description.fil
Fil: Ward, P. A.. Mullard Space Science Laboratory; Reino Unido
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Fil: Fiore, F.. Osservatorio Astronomico di Roma; Italia
dc.description.fil
Fil: Vergani, S. D.. Dublin Institute for Advanced Studies; Irlanda
dc.description.fil
Fil: D'Elia, V.. Osservatorio Astronomico di Roma; Italia
dc.description.fil
Fil: Krongold, Y.. Universidad Nacional Autónoma de México; México
dc.description.fil
Fil: Nicastro, F.. Osservatorio Astronomico di Roma; Italia
dc.description.fil
Fil: Meurs, E. J. A.. Dublin City University; Irlanda
dc.description.fil
Fil: Chincarini, G.. Osservatorio Astronomico di Brera; Italia
dc.description.fil
Fil: Covino, S.. Osservatorio Astronomico di Brera; Italia
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Fil: Della Valle, M.. Osservatorio Astronomico di Capodimonte; Italia
dc.description.fil
Fil: Fugazza, D.. Osservatorio Astronomico di Brera; Italia
dc.description.fil
Fil: Norci, L.. Dublin Institute for Advanced Studies; Irlanda
dc.description.fil
Fil: Sbordone, L.. Centre National de la Recherche Scientifique. Observatoire de Paris; Francia
dc.description.fil
Fil: Stella, L.. Osservatorio Astronomico di Roma; Italia
dc.description.fil
Fil: Tagliaferri, G.. Osservatorio Astronomico di Brera; Italia
dc.description.fil
Fil: Burrows, D. N.. University of Pennsylvania; Estados Unidos
dc.description.fil
Fil: Gehrels, N.. National Aeronautics And Space Administration; Estados Unidos
dc.description.fil
Fil: Goldoni, P.. Laboratoire Astroparticule et Cosmologie; Francia
dc.description.fil
Fil: Malesani, D.. Niels Bohr Institute; Dinamarca
dc.description.fil
Fil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
dc.description.fil
Fil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
dc.description.fil
Fil: Perna, R.. State University Of Colorado Boulder; Estados Unidos
dc.journal.title
Astronomy and Astrophysics
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361:20079015
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2008/48/aa9015-07/aa9015-07.html
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/0811.0989
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