| dc.date.accessioned | 2020-03-11T20:35:59Z | |
| dc.date.accessioned | 2022-10-18T23:02:24Z | |
| dc.date.available | 2020-03-11T20:35:59Z | |
| dc.date.available | 2022-10-18T23:02:24Z | |
| dc.date.created | 2020-03-11T20:35:59Z | |
| dc.date.issued | 2010 | |
| dc.identifier | http://hdl.handle.net/10533/240822 | |
| dc.identifier | 15010003 | |
| dc.identifier | WOS:000273981100044 | |
| dc.identifier | no scielo | |
| dc.identifier | eid=2-s2.0-75749134949 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4472161 | |
| dc.description.abstract | Long duration gamma-ray bursts (GRBs) mark the explosive death of some massive stars and are a rare sub-class of Type Ibc supernovae (SNe Ibc). They are distinguished by the production of an energetic and collimated relativistic outflow powered by a centr | |
| dc.language | eng | |
| dc.relation | https://doi.org/10.1038/nature08714 | |
| dc.relation | 10.1038/nature08714 | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
| dc.title | A Relativistic Type Ibc Supernova Without a Detected Gamma-ray Burst | |
| dc.type | Articulo | |
