Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/24890
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Burlon, D. | en_US |
dc.contributor.author | Murphy, T. | en_US |
dc.contributor.author | GHIRLANDA, Giancarlo | en_US |
dc.contributor.author | Hancock, P. J. | en_US |
dc.contributor.author | Parry, R. | en_US |
dc.contributor.author | SALVATERRA, Ruben | en_US |
dc.date.accessioned | 2020-05-15T15:11:22Z | - |
dc.date.available | 2020-05-15T15:11:22Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24890 | - |
dc.description.abstract | Current models suggest gamma-ray bursts could be used as a way of probing Population-III stars - the first stars in the early Universe. In this paper, we use numerical simulations to demonstrate that late-time radio observations of gamma-ray burst afterglows could provide a means of identifying bursts that originate from Population-III stars, if these were highly massive, independently from their redshift. We then present the results from a pilot study using the Australia Telescope Compact Array at 17 GHz, designed to test the hypothesis that there may be Population-III gamma-ray bursts amongst the current sample of known events. We observed three candidates plus a control gamma-ray burst, and make no detections with upper limits of 20-40 μJy at 500-1300 d post-explosion. | en_US |
dc.language.iso | eng | en_US |
dc.title | Gamma-ray bursts from massive Population-III stars: clues from the radio band | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw905 | en_US |
dc.identifier.scopus | 2-s2.0-84975045817 | en_US |
dc.identifier.isi | 000379840900081 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/459/3/3356/2595257 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 459 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 3356 | en_US |
dc.relation.lastpage | 3362 | en_US |
dc.relation.numberofpages | 8 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016MNRAS.459.3356B | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-5876-9259 | - |
crisitem.author.orcid | 0000-0002-9393-8078 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
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stw905.pdf | PDF editoriale | 1.29 MB | Adobe PDF | Visualizza/apri |
1604.03946.pdf | postprint | 2.87 MB | Adobe PDF | Visualizza/apri |
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