Simultaneous detection of an intrinsic absorber and a compact jet emission in the X-ray binary IGR J17091-3624 during a hard accretion state
dc.contributor.author | Gatuzz, E. | |
dc.contributor.author | Díaz Trigo, M. | |
dc.contributor.author | Miller-Jones, James | |
dc.contributor.author | Migliari, S. | |
dc.date.accessioned | 2023-04-18T14:58:21Z | |
dc.date.available | 2023-04-18T14:58:21Z | |
dc.date.issued | 2020 | |
dc.identifier.citation | Gatuzz, E. and Díaz Trigo, M. and Miller-Jones, J.C.A. and Migliari, S. 2020. Simultaneous detection of an intrinsic absorber and a compact jet emission in the X-ray binary IGR J17091-3624 during a hard accretion state. Monthly Notices of the Royal Astronomical Society. 491 (4): pp. 4857-4868. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/91532 | |
dc.identifier.doi | 10.1093/mnras/stz3385 | |
dc.description.abstract |
We present a detailed analysis of three XMM-Newton observations of the black hole low-mass X-ray binary IGR J17091-3624 taken during its 2016 outburst. Radio observations obtained with the Australia Telescope Compact Array indicate the presence of a compact jet during all observations. From the best X-ray data fit results, we concluded that the observations were taken during a transition from a hard accretion state to a hard-intermediate accretion state. For Observations 1 and 2, a local absorber can be identified in the EPIC-pn spectra but not in the RGS spectra, preventing us from distinguishing between absorption local to the source and that from the hot ISM component. For Observation 3, on the other hand, we have identified an intrinsic ionized static absorber in both EPIC-pn and RGS spectra. The absorber, observed simultaneously with a compact jet emission, is characterized by an ionization parameter of 1.96 < log ζ < 2.05 and traced mainly by Ne x, Mg xii, Si xiii, and Fe xviii. | |
dc.language | English | |
dc.publisher | OXFORD UNIV PRESS | |
dc.relation.sponsoredby | http://purl.org/au-research/grants/arc/FT140101082 | |
dc.subject | Science & Technology | |
dc.subject | Physical Sciences | |
dc.subject | Astronomy & Astrophysics | |
dc.subject | accretion, accretion discs | |
dc.subject | black hole physics | |
dc.subject | X-rays: binaries | |
dc.subject | X-rays: individual: IGR J17091-3624 | |
dc.subject | GRS 1915+105 | |
dc.subject | DISK WIND | |
dc.subject | SPECTRA | |
dc.subject | CHANDRA | |
dc.subject | MODEL | |
dc.subject | GAS | |
dc.subject | PHOTOIONIZATION | |
dc.subject | SPECTROSCOPY | |
dc.subject | INSTABILITY | |
dc.subject | STABILITY | |
dc.title | Simultaneous detection of an intrinsic absorber and a compact jet emission in the X-ray binary IGR J17091-3624 during a hard accretion state | |
dc.type | Journal Article | |
dcterms.source.volume | 491 | |
dcterms.source.number | 4 | |
dcterms.source.startPage | 4857 | |
dcterms.source.endPage | 4868 | |
dcterms.source.issn | 0035-8711 | |
dcterms.source.title | Monthly Notices of the Royal Astronomical Society | |
dc.date.updated | 2023-04-18T14:58:20Z | |
curtin.note |
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. (c) 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | |
curtin.department | School of Elec Eng, Comp and Math Sci (EECMS) | |
curtin.accessStatus | Open access | |
curtin.faculty | Faculty of Science and Engineering | |
curtin.contributor.orcid | Miller-Jones, James [0000-0003-3124-2814] | |
curtin.contributor.researcherid | Miller-Jones, James [B-2411-2013] | |
dcterms.source.eissn | 1365-2966 | |
curtin.contributor.scopusauthorid | Miller-Jones, James [10044231400] | |
curtin.repositoryagreement | V3 |