Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31865
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Coti Zelati, F. | en_US |
dc.contributor.author | Borghese, A. | en_US |
dc.contributor.author | ISRAEL, Gian Luca | en_US |
dc.contributor.author | Rea, N. | en_US |
dc.contributor.author | Esposito, P. | en_US |
dc.contributor.author | PILIA, Maura | en_US |
dc.contributor.author | BURGAY, MARTA | en_US |
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.contributor.author | CORONGIU, ALESSANDRO | en_US |
dc.contributor.author | RIDOLFI, ALESSANDRO | en_US |
dc.contributor.author | Dehman, C. | en_US |
dc.contributor.author | Viganò, D. | en_US |
dc.contributor.author | Turolla, R. | en_US |
dc.contributor.author | Zane, S. | en_US |
dc.contributor.author | Tiengo, A. | en_US |
dc.contributor.author | Keane, E. F. | en_US |
dc.date.accessioned | 2022-03-24T11:51:56Z | - |
dc.date.available | 2022-03-24T11:51:56Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31865 | - |
dc.description.abstract | The detection of a short hard X-ray burst and an associated bright soft X-ray source by the Swift satellite in 2020 October heralded a new magnetar in outburst, SGR J1830-0645. Pulsations at a period of ∼10.4 s were detected in prompt follow-up X-ray observations. We present here the analysis of the Swift/Burst Alert Telescope burst, of XMM-Newton and the Nuclear Spectroscopic Telescope Array observations performed at the outburst peak, and of a Swift/X-ray Telescope monitoring campaign over the subsequent month. The burst was single-peaked, lasted ∼6 ms, and released a fluence of ≍5 × 10<SUP>-9</SUP> erg cm<SUP>-2</SUP> (15-50 keV). The spectrum of the X-ray source at the outburst peak was well described by an absorbed double-blackbody model plus a power-law component detectable up to ∼25 keV. The unabsorbed X-ray flux decreased from ∼5 × 10<SUP>-11</SUP> to ∼2.5 × 10<SUP>-11</SUP> erg cm<SUP>-2</SUP> s<SUP>-1</SUP> one month later (0.3-10 keV). Based on our timing analysis, we estimate a dipolar magnetic field ≍5.5 × 10<SUP>14</SUP> G at pole, a spin-down luminosity ≍2.4 × 10<SUP>32</SUP> erg s<SUP>-1</SUP>, and a characteristic age ≍24 kyr. The spin modulation pattern appears highly pulsed in the soft X-ray band, and becomes smoother at higher energies. Several short X-ray bursts were detected during our campaign. No evidence for periodic or single-pulse emission was found at radio frequencies in observations performed with the Sardinia Radio Telescope and Parkes. According to magneto-thermal evolutionary models, the real age of SGR J1830-0645 is close to the characteristic age, and the dipolar magnetic field at birth was slightly larger, ∼10<SUP>15</SUP> G. | en_US |
dc.language.iso | eng | en_US |
dc.title | The New Magnetar SGR J1830-0645 in Outburst | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/2041-8213/abda52 | en_US |
dc.identifier.scopus | 2-s2.0-85100771764 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/2041-8213/abda52 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85100771764 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 907 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | L34 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL LETTERS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021ApJ...907L..34C | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | 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. Roma | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0001-5480-6438 | - |
crisitem.author.orcid | 0000-0001-7397-8091 | - |
crisitem.author.orcid | 0000-0002-8265-4344 | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
crisitem.author.orcid | 0000-0002-5924-3141 | - |
crisitem.author.orcid | 0000-0001-6762-2638 | - |
crisitem.journal.journalissn | 2041-8205 | - |
crisitem.journal.ance | E196528 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2011.08653.pdf | preprint | 2.84 MB | Adobe PDF | View/Open |
Zelati_2021_ApJL_907_L34.pdf | [Administrators only] | 2 MB | Adobe PDF |
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