Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31849
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | DELLA VALLE, Massimo | en_US |
dc.contributor.author | Guetta, D. | en_US |
dc.contributor.author | CAPPELLARO, Enrico | en_US |
dc.contributor.author | AMATI, LORENZO | en_US |
dc.contributor.author | BOTTICELLA, MARIA TERESA | en_US |
dc.contributor.author | Branchesi, M. | en_US |
dc.contributor.author | BROCATO, Enzo | en_US |
dc.contributor.author | Izzo, L. | en_US |
dc.contributor.author | Perez-Torres, M. A. | en_US |
dc.contributor.author | STRATTA, MARIA GIULIANA | en_US |
dc.date.accessioned | 2022-03-24T10:23:34Z | - |
dc.date.available | 2022-03-24T10:23:34Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31849 | - |
dc.description.abstract | We compute the local rate of events similar to GRB 170817A, which has been recently found to be associated with a kilonova (KN) outburst. Our analysis finds an observed rate of such events of R_KN∼ 352^{+810}_{-281} Gpc<SUP>-3</SUP> yr<SUP>-1</SUP>. After comparing at their face values this density of sGRB outbursts with the much higher density of binary neutron star (BNS) mergers of 1540^{+3200}_{-1220} Gpc<SUP>-3</SUP> yr<SUP>-1</SUP>, estimated by LIGO-Virgo collaboration, one can conclude, admittedly with large uncertainty that either only a minor fraction of BNS mergers produces short gamma-ray bursts (sGRB)/KN events or the sGRBs associated with BNS mergers are beamed and observable under viewing angles as large as θ ≲ 40°. Finally, we provide preliminary estimates of the number of sGRB/KN events detected by future surveys carried out with present/future ground-based/space facilities, such as LSST, VST, ZTF, SKA, and THESEUS. | en_US |
dc.language.iso | eng | en_US |
dc.title | GW170817: implications for the local kilonova rate and for surveys from ground-based facilities | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty2541 | en_US |
dc.identifier.scopus | 2-s2.0-85054751065 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/481/4/4355/5101464?login=true | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 481 | en_US |
dc.relation.issue | 4 | en_US |
dc.relation.firstpage | 4355 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | ISR | 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 | 2018MNRAS.481.4355D | 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.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | O.A. Abruzzo | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0003-3142-5020 | - |
crisitem.author.orcid | 0000-0001-5008-8619 | - |
crisitem.author.orcid | 0000-0001-5355-7388 | - |
crisitem.author.orcid | 0000-0002-3938-692X | - |
crisitem.author.orcid | 0000-0001-7988-8177 | - |
crisitem.author.orcid | 0000-0003-1055-7980 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
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1809.04295.pdf | preprint | 402.16 kB | Adobe PDF | Visualizza/apri |
sty2541.pdf | Pdf editoriale | 292.2 kB | Adobe PDF | Visualizza/apri |
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