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Campo DC | Valor | Idioma |
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dc.rights.license | Copyright © 2020, Oxford University Press | - |
dc.contributor.author | Parker, M. L. | - |
dc.contributor.author | Matzeu, G. A. | - |
dc.contributor.author | Alston, W. N. | - |
dc.contributor.author | Fabian, A. C. | - |
dc.contributor.author | Lobban, A. | - |
dc.contributor.author | Miniutti, G. | - |
dc.contributor.author | Pinto, C. | - |
dc.contributor.author | Santos Lleó, M. | - |
dc.contributor.author | Schartel, N. | - |
dc.contributor.other | Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737 | - |
dc.date.accessioned | 2021-04-09T10:37:11Z | - |
dc.date.available | 2021-04-09T10:37:11Z | - |
dc.date.issued | 2020-08-25 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society: Letters 498(1): L140-L144(2020) | es |
dc.identifier.issn | 1745-3925 | - |
dc.identifier.other | https://academic.oup.com/mnrasl/article-abstract/498/1/L140/5896962 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12666/196 | - |
dc.description | This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model) | es |
dc.description.abstract | We present joint NuSTAR and XMM–Newton observations of the bright, variable quasar IRAS 13349+2438. This combined data set shows two clear iron absorption lines at 8 and 9 keV, which are most likely associated with two layers of mildly relativistic blueshifted absorption, with velocities of ∼0.14c and ∼0.27c. We also find strong evidence for a series of Ly α absorption lines at intermediate energies in a stacked XMM–Newton EPIC-pn spectrum, at the same blueshift as the lower velocity iron feature. This is consistent with a scenario where an outflowing wind is radially stratified, so faster, higher ionization material is observed closer to the black hole, and cooler, slower material is seen from streamlines at larger radii. | es |
dc.description.sponsorship | MLP and GM are supported by European Space Agency (ESA) research fellowships. This letter was written during the 2020 Covid19 outbreak. The authors would like to thank the medical staff of our respective countries for their work fighting the global pandemic. We thank the referee, James Reeves, for detailed and constructive feedback; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737). | es |
dc.language.iso | eng | es |
dc.publisher | Oxford Academics: Blackwell Publishing | es |
dc.subject | Accretion | es |
dc.subject | Accretion Disc | es |
dc.subject | Black Hole Physics | es |
dc.subject | Galaxies: active | es |
dc.title | Detection of a possible multiphase ultra-fast outflow in IRAS 13349+2438 with NuSTAR and XMM-Newton. | es |
dc.type | info:eu-repo/semantics/article | es |
dc.contributor.orcid | 0000-0002-5635-5340 | - |
dc.contributor.orcid | 0000-0003-1994-5322 | - |
dc.contributor.orcid | 0000-0003-2658-6559 | - |
dc.contributor.orcid | 0000-0001-5948-8360 | - |
dc.contributor.orcid | 0000-0003-2532-7379 | - |
dc.contributor.orcid | 0000-0002-9378-4072 | - |
dc.identifier.doi | 10.1093/mnrasl/slaa144 | - |
dc.identifier.e-issn | 1745-3933 | - |
dc.contributor.funder | European Space Agency (ESA) | - |
dc.description.peerreviewed | Peer review | es |
dc.type.hasVersion | info:eu-repo/semantics/publishedVersion | - |
dc.rights.accessRights | info:eu-repo/semantics/restrictedAccess | - |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | - |
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