Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26720
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | De Pasquale, Massimiliano | en_US |
dc.contributor.author | Page, Mathew | en_US |
dc.contributor.author | Kann, David | en_US |
dc.contributor.author | Oates, Samantha | en_US |
dc.contributor.author | Schulze, Steve | en_US |
dc.contributor.author | Zhang, Bing | en_US |
dc.contributor.author | Cano, Zach | en_US |
dc.contributor.author | Gendre, Bruce | en_US |
dc.contributor.author | Malesani, Daniele | en_US |
dc.contributor.author | ROSSI, Andrea | en_US |
dc.contributor.author | Gehrels, Neil | en_US |
dc.contributor.author | Troja, Eleonora | en_US |
dc.contributor.author | PIRO, LUIGI | en_US |
dc.contributor.author | Boër, Michel | en_US |
dc.contributor.author | STRATTA, MARIA GIULIANA | en_US |
dc.date.accessioned | 2020-08-19T11:16:23Z | - |
dc.date.available | 2020-08-19T11:16:23Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 2075-4434 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26720 | - |
dc.description.abstract | GRB 130427A was the most luminous gamma-ray burst detected in the last 30 years. With an isotropic energy output of <mml:math display="inline"> <mml:mrow> <mml:mn>8.5</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mn>53</mml:mn> </mml:msup> </mml:mrow> </mml:math> erg and redshift of 0.34, it combined very high energetics with a relative proximity to Earth in an unprecedented way. Sensitive X-ray observatories such as XMM-Newton and Chandra have detected the afterglow of this event for a record-breaking baseline longer than 80 million seconds. The light curve displays a simple power-law over more than three decades in time. In this presentation, we explore the consequences of this result for a few models put forward so far to interpret GRB 130427A, and more in general the implication of this outcome in the context of the standard forward shock model. | en_US |
dc.language.iso | eng | en_US |
dc.title | Challenging the Forward Shock Model with the 80 Ms Follow up of the X-ray Afterglow of Gamma-Ray Burst 130427A | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3390/galaxies5010006 | en_US |
dc.identifier.scopus | 2-s2.0-85030852771 | en_US |
dc.identifier.isi | 000398779500006 | en_US |
dc.identifier.url | https://www.mdpi.com/2075-4434/5/1/6 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 5 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 6 | en_US |
dc.relation.lastpage | 13 | en_US |
dc.relation.numberofpages | 7 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | ISL | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | GALAXIES | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017Galax...5....6D | 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.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 2075-4434 | - |
crisitem.journal.ance | E222261 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0002-8860-6538 | - |
crisitem.author.orcid | 0000-0003-4159-3984 | - |
crisitem.author.orcid | 0000-0003-1055-7980 | - |
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