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http://hdl.handle.net/20.500.12386/27007
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Pintore, Fabio | en_US |
dc.contributor.author | MEREGHETTI, Sandro | en_US |
dc.contributor.author | TIENGO, ANDREA | en_US |
dc.contributor.author | Vianello, Giacomo | en_US |
dc.contributor.author | Costantini, Elisa | en_US |
dc.contributor.author | ESPOSITO, PAOLO | en_US |
dc.date.accessioned | 2020-08-31T16:54:30Z | - |
dc.date.available | 2020-08-31T16:54:30Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27007 | - |
dc.description.abstract | A bright burst, followed by an X-ray tail lasting ∼10 ks, was detected during an XMM-Newton observation of the magnetar 1E 1547.0-5408 carried out on 2009 February 3. The burst, also observed by Swift/BAT, had a spectrum well fitted by the sum of two blackbodies with temperatures of ∼4 and 10 keV and a fluence in the 0.3-150 keV energy range of ∼10<SUP>-5</SUP> erg cm<SUP>-2</SUP>. The X-ray tail had a fluence of ∼4 × 10<SUP>-8</SUP> erg cm<SUP>-2</SUP>. Thanks to the knowledge of the distances and relative optical depths of three dust clouds between us and 1E 1547.0-5408, we show that most of the X-rays in the tail can be explained by dust scattering of the burst emission, except for the first ∼20-30 s. We point out that other X-ray tails observed after strong magnetar bursts may contain a non-negligible contribution due to dust scattering. | en_US |
dc.language.iso | eng | en_US |
dc.title | The effect of X-ray dust scattering on a bright burst from the magnetar 1E 1547.0-5408 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx368 | en_US |
dc.identifier.scopus | 2-s2.0-85052513660 | en_US |
dc.identifier.isi | 000398419400073 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/467/3/3467/2982882 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 467 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 3467 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | DEU | 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 | 2017MNRAS.467.3467P | 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 | IASF Palermo | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0002-3869-2925 | - |
crisitem.author.orcid | 0000-0003-3259-7801 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
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