Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/29013
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Nowak, Michael A. | en_US |
dc.contributor.author | PAIZIS, ADAMANTIA | en_US |
dc.contributor.author | Jaisawal, Gaurava Kumar | en_US |
dc.contributor.author | Chenevez, Jérôme | en_US |
dc.contributor.author | Chaty, Sylvain | en_US |
dc.contributor.author | Fortin, Francis | en_US |
dc.contributor.author | Rodriguez, Jérôme | en_US |
dc.contributor.author | Wilms, Jörn | en_US |
dc.date.accessioned | 2020-12-18T12:28:14Z | - |
dc.date.available | 2020-12-18T12:28:14Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29013 | - |
dc.description.abstract | An accreting millisecond X-ray pulsar, IGR J17591-2342 was discovered in 2018 August in scans of the Galactic bulge and center by the International Gamma-Ray Astrophysics Laboratory X-ray and gamma-ray observatory. It exhibited an unusual outburst profile with multiple peaks in the X-ray, as observed by several X-ray satellites over 3 months. Here we present observations of this source performed in the X-ray/gamma-ray and near-infrared domains and focus on a simultaneous observation performed with the Chandra High Energy Transmission Gratings Spectrometer (HETGS) and the Neutron Star Interior Composition Explorer (NICER). The HETGS provides high-resolution spectra of the Si edge region that yield clues as to the source’s distance and reveal evidence (at 99.999% significance) of an outflow with a velocity of 2800 km s<SUP>-1</SUP>. We demonstrate good agreement between the NICER and HETGS continua, provided that one properly accounts for the differing manners in which these instruments view the dust-scattering halo in the source’s foreground. Unusually, we find a possible set of Ca lines in the HETGS spectra (with significances ranging from 97.0% to 99.7%). We hypothesize that IGR J17591-2342 is a neutron star low-mass X-ray binary at the distance of the Galactic bulge or beyond that may have formed from the collapse of a white dwarf system in a rare, calcium-rich Type Ib supernova explosion. | en_US |
dc.language.iso | eng | en_US |
dc.title | Chandra-HETGS Characterization of an Outflowing Wind in the Accreting Millisecond Pulsar IGR J17591-2342 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/ab0a71 | en_US |
dc.identifier.scopus | 2-s2.0-85064439864 | en_US |
dc.identifier.isi | 000462602500002 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/ab0a71 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 874 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 69 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 8 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | DNK | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019ApJ...874...69N | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_10 High energy and particle astronomy – X-rays, cosmic rays, gamma rays, neutrinos | 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.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-5067-0377 | - |
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