Long gamma-ray bursts and core-collapse supernovae have different environments

dc.creatorFruchter, A. S.
dc.creatorLevan, A. J.
dc.creatorStrolger, L.
dc.creatorVreeswijk, P. M.
dc.creatorThorsett, S. E.
dc.creatorBersier, D.
dc.creatorBurud, I.
dc.creatorCerón, J. M. Castro
dc.creatorCastro-Tirado, A. J.
dc.creatorConselice, C.
dc.creatorDahlen, T.
dc.creatorFerguson, H. C.
dc.creatorFynbo, J. P. U.
dc.creatorGarnavich, P. M.
dc.creatorGibbons, R. A.
dc.creatorGorosabel, J.
dc.creatorGull, T. R.
dc.creatorHjorth, J.
dc.creatorHolland, S. T.
dc.creatorKouveliotou, C.
dc.creatorLevay, Z.
dc.creatorLivio, M.
dc.creatorMetzger, M. R.
dc.creatorNugent, P. E.
dc.creatorPetro, L.
dc.creatorPian, E.
dc.creatorRhoads, J. E.
dc.creatorRiess, A. G.
dc.creatorSahu, K. C.
dc.creatorSmette, A.
dc.creatorTanvir, N. R.
dc.creatorWijers, R. A. M. J.
dc.creatorWoosley, S. E.
dc.date2006-03-20
dc.date2006-05-05
dc.date.accessioned2026-07-07T11:57:20Z
dc.date.available2026-07-07T11:57:20Z
dc.descriptionWhen massive stars exhaust their fuel they collapse and often produce the extraordinarily bright explosions known as core-collapse supernovae. On occasion, this stellar collapse also powers an even more brilliant relativistic explosion known as a long-duration gamma-ray burst. One would then expect that long gamma-ray bursts and core-collapse supernovae should be found in similar galactic environments. Here we show that this expectation is wrong. We find that the long gamma-ray bursts are far more concentrated on the very brightest regions of their host galaxies than are the core-collapse supernovae. Furthermore, the host galaxies of the long gamma-ray bursts are significantly fainter and more irregular than the hosts of the core-collapse supernovae. Together these results suggest that long-duration gamma-ray bursts are associated with the most massive stars and may be restricted to galaxies of limited chemical evolution. Our results directly imply that long gamma-ray bursts are relatively rare in galaxies such as our own Milky Way.
dc.description27 pages, 4 figures, submitted to Nature on 22 August 2005, revised 9 February 2006, online publication 10 May 2006. Supplementary material referred to in the text can be found at http://www.stsci.edu/~fruchter/GRB/locations/supplement.pdf . This new version contains minor changes to match the final published version
dc.identifierhttps://arxiv.org/abs/astro-ph/0603537
dc.identifierhttp://arxiv.org/abs/astro-ph/0603537
dc.identifierNature441:463-468,2006
dc.identifierdoi:10.1038/nature04787
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205848
dc.subjectAstrophysics
dc.titleLong gamma-ray bursts and core-collapse supernovae have different environments
dc.typetext

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