Long gamma-ray bursts and core-collapse supernovae have different environments
| dc.creator | Fruchter, A. S. | |
| dc.creator | Levan, A. J. | |
| dc.creator | Strolger, L. | |
| dc.creator | Vreeswijk, P. M. | |
| dc.creator | Thorsett, S. E. | |
| dc.creator | Bersier, D. | |
| dc.creator | Burud, I. | |
| dc.creator | Cerón, J. M. Castro | |
| dc.creator | Castro-Tirado, A. J. | |
| dc.creator | Conselice, C. | |
| dc.creator | Dahlen, T. | |
| dc.creator | Ferguson, H. C. | |
| dc.creator | Fynbo, J. P. U. | |
| dc.creator | Garnavich, P. M. | |
| dc.creator | Gibbons, R. A. | |
| dc.creator | Gorosabel, J. | |
| dc.creator | Gull, T. R. | |
| dc.creator | Hjorth, J. | |
| dc.creator | Holland, S. T. | |
| dc.creator | Kouveliotou, C. | |
| dc.creator | Levay, Z. | |
| dc.creator | Livio, M. | |
| dc.creator | Metzger, M. R. | |
| dc.creator | Nugent, P. E. | |
| dc.creator | Petro, L. | |
| dc.creator | Pian, E. | |
| dc.creator | Rhoads, J. E. | |
| dc.creator | Riess, A. G. | |
| dc.creator | Sahu, K. C. | |
| dc.creator | Smette, A. | |
| dc.creator | Tanvir, N. R. | |
| dc.creator | Wijers, R. A. M. J. | |
| dc.creator | Woosley, S. E. | |
| dc.date | 2006-03-20 | |
| dc.date | 2006-05-05 | |
| dc.date.accessioned | 2026-07-07T11:57:20Z | |
| dc.date.available | 2026-07-07T11:57:20Z | |
| dc.description | When 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.description | 27 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.identifier | https://arxiv.org/abs/astro-ph/0603537 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0603537 | |
| dc.identifier | Nature441:463-468,2006 | |
| dc.identifier | doi:10.1038/nature04787 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/205848 | |
| dc.subject | Astrophysics | |
| dc.title | Long gamma-ray bursts and core-collapse supernovae have different environments | |
| dc.type | text |