Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28622
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Borghese, A. | en_US |
dc.contributor.author | Coti Zelati, F. | en_US |
dc.contributor.author | Esposito, P. | en_US |
dc.contributor.author | Rea, N. | en_US |
dc.contributor.author | DE LUCA, Andrea | en_US |
dc.contributor.author | BACHETTI, Matteo | en_US |
dc.contributor.author | ISRAEL, Gian Luca | en_US |
dc.contributor.author | Perna, R. | en_US |
dc.contributor.author | Pons, J. A. | en_US |
dc.date.accessioned | 2020-12-02T11:22:44Z | - |
dc.date.available | 2020-12-02T11:22:44Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28622 | - |
dc.description.abstract | We report on a new NuSTAR observation and on the ongoing Swift X-Ray Telescope monitoring campaign of the peculiar source 1E 161348-5055, located at the centre of the supernova remnant RCW 103, which is recovering from its last outburst in 2016 June. The X-ray spectrum at the epoch of the NuSTAR observation can be described by either two absorbed blackbodies (kT_BB_1 ∼ 0.5 keV, kT_BB_2 ∼ 1.2 keV) or an absorbed blackbody plus a power law (kT_BB_1 ∼ 0.6 keV, Γ ∼ 3.9). The observed flux was ∼9 × 10<SUP>-12</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, ∼3 times lower than what observed at the outburst onset, but about one order of magnitude higher than the historical quiescent level. A periodic modulation was detected at the known 6.67 h periodicity. The spectral decomposition and evolution along the outburst decay are consistent with 1E 161348-5055 being a magnetar, the slowest ever detected. | en_US |
dc.language.iso | eng | en_US |
dc.title | Gazing at the ultraslow magnetar in RCW 103 with NuSTAR and Swift | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty1119 | en_US |
dc.identifier.scopus | 2-s2.0-85048510888 | en_US |
dc.identifier.isi | 000439501300055 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/478/1/741/4990953 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 478 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 741 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 9 | en_US |
dc.description.international | sì | 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.478..741B | 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 Milano | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0001-6739-687X | - |
crisitem.author.orcid | 0000-0002-4576-9337 | - |
crisitem.author.orcid | 0000-0001-5480-6438 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
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sty1119.pdf | Pdf editoriale | 7.14 MB | Adobe PDF | Visualizza/apri |
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