Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27085
Campo DC | Valore | Lingua |
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dc.contributor.author | Troja, E. | - |
dc.contributor.author | Ryan, G. | - |
dc.contributor.author | PIRO, LUIGI | - |
dc.contributor.author | van Eerten, H. | - |
dc.contributor.author | Cenko, S. B. | - |
dc.contributor.author | Yoon, Y. | - |
dc.contributor.author | Lee, S.-K. | - |
dc.contributor.author | Im, M. | - |
dc.contributor.author | Sakamoto, T. | - |
dc.contributor.author | Gatkine, P. | - |
dc.contributor.author | Kutyrev, A. | - |
dc.contributor.author | Veilleux, S. | - |
dc.date.accessioned | 2020-09-03T10:22:44Z | - |
dc.date.available | 2020-09-03T10:22:44Z | - |
dc.date.issued | 2018 | - |
dc.identifier.issn | 2041-1723 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27085 | - |
dc.description.abstract | The recent discovery of a gamma-ray burst (GRB) coincident with the gravitational-wave (GW) event GW170817 revealed the existence of a population of low-luminosity short duration gamma-ray transients produced by neutron star mergers in the nearby Universe. These events could be routinely detected by existing gamma-ray monitors, yet previous observations failed to identify them without the aid of GW triggers. Here we show that GRB150101B is an analogue of GRB170817A located at a cosmological distance. GRB150101B is a faint short burst characterized by a bright optical counterpart and a long-lived X-ray afterglow. These properties are unusual for standard short GRBs and are instead consistent with an explosion viewed off-axis: the optical light is produced by a luminous kilonova, while the observed X-rays trace the GRB afterglow viewed at an angle of 13°. Our findings suggest that these properties could be common among future electromagnetic counterparts of GW sources. | - |
dc.language.iso | eng | - |
dc.title | A luminous blue kilonova and an off-axis jet from a compact binary merger at z = 0.1341 | - |
dc.type | Article | - |
dc.identifier.doi | 10.1038/s41467-018-06558-7 | en_US |
dc.identifier.scopus | 2-s2.0-85055079407 | en_US |
dc.identifier.isi | 000447360700001 | en_US |
dc.identifier.url | https://www.nature.com/articles/s41467-018-06558-7 | - |
dc.relation.medium | ELETTRONICO | - |
dc.relation.volume | 9 | - |
dc.relation.issue | 1 | - |
dc.relation.firstpage | 4089 | - |
dc.type.referee | REF_1 | - |
dc.description.international | sì | - |
dc.contributor.country | ITA | - |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | - |
dc.relation.journal | NATURE COMMUNICATIONS | - |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018NatCo...9.4089T | - |
dc.description.apc | no | - |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 2041-1723 | - |
crisitem.journal.ance | E203533 | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0003-4159-3984 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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s41467-018-06558-7.pdf | Pdf editoriale | 1.58 MB | Adobe PDF | Visualizza/apri |
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