The Galaxy Density Environment of Gamma-Ray Burst Host Galaxies

We analyze cross-correlation functions between gamma-ray burst (GRB) hosts and surrounding galaxies. We have used data obtained with the Very Large Telescope at Cerro Paranal (Chile), as well as public Hubble Space Telescope data. Our results indicate that GRB host galaxies do not reside in high gal...

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Published inThe Astrophysical journal Vol. 614; no. 1; pp. 84 - 90
Main Authors Bornancini, Carlos G, Martínez, Héctor J, Lambas, Diego G, Le Floc’h, Emeric, Mirabel, I. Félix, Minniti, Dante
Format Journal Article
LanguageEnglish
Published Chicago, IL IOP Publishing 10.10.2004
University of Chicago Press
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Summary:We analyze cross-correlation functions between gamma-ray burst (GRB) hosts and surrounding galaxies. We have used data obtained with the Very Large Telescope at Cerro Paranal (Chile), as well as public Hubble Space Telescope data. Our results indicate that GRB host galaxies do not reside in high galaxy density environments. Moreover, the host galaxy-galaxy cross-correlations show a relatively low amplitude. Our results are in agreement with the cross-correlation function between star forming galaxies and surrounding objects in the Hubble Deep Field-North (HDF-N).
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
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ISSN:0004-637X
1538-4357
DOI:10.1086/392497