Signatures of feedback in the spectacular extended emission region of NGC 5972
dc.catalogador | dfo | |
dc.contributor.author | Harvey, Thomas | |
dc.contributor.author | Maksym, W. Peter | |
dc.contributor.author | Keel, William | |
dc.contributor.author | Koss, Michael | |
dc.contributor.author | Bennert, Vardha N. | |
dc.contributor.author | Chojnowski, S. Drew | |
dc.contributor.author | Treister, Ezequiel | |
dc.contributor.author | Finlez, Carolina | |
dc.contributor.author | Lintott, Chris J. | |
dc.contributor.author | Moiseev, Alexei | |
dc.contributor.author | Simmons, Brooke D. | |
dc.contributor.author | Sartori, Lia F. | |
dc.contributor.author | Urry, Megan | |
dc.date.accessioned | 2023-12-06T20:47:12Z | |
dc.date.available | 2023-12-06T20:47:12Z | |
dc.date.issued | 2023 | |
dc.description.abstract | We present Chandra X-ray Observatory observations and Space Telescope Imaging Spectrograph spectra of NGC 5972, one of the 19 ‘Voorwerpjes’ galaxies. This galaxy contains an extended emission-line region (EELR) and an arcsecond scale nuclear bubble. NGC 5972 is a faded active galactic nucleus (AGN), with EELR luminosity suggesting a 2.1 dex decrease in Lbol in the last ∼5 × 104 yr. We investigate the role of AGN feedback in exciting the EELR and bubble given the long-term variability and potential accretion state changes. We detect broad-band (0.3–8 keV) X-ray emission in the near-nuclear regions, coincident with the [O III] bubble, as well as diffuse soft X-ray emission coincident with the EELR. The soft nuclear (0.5–1.5 keV) emission is spatially extended and the spectra are consistent with two APEC thermal populations (∼0.80 and ∼0.10 keV). We find a bubble age >2.2 Myr, suggesting formation before the current variability. We find evidence for efficient feedback with Pkin/Lbol ∼ 0.8 per cent, which may be overestimated given the recent Lbol variation. [O III] kinematics show a 300 km s−1 high-ionization velocity consistent with disturbed rotation or potentially the line-of-sight component of a ∼780 km s−1 thermal X-ray outflow capable of driving strong shocks to photoionize the precursor material. We explore possibilities to explain the overall jet, radio lobe and EELR misalignment including evidence for a double supermassive black hole which could support a complex misaligned system. | |
dc.description.funder | Center for Astrophysics | |
dc.description.funder | Chandra Source Catalog | |
dc.description.funder | Chandra X-ray Center | |
dc.description.funder | National Science Foundation | |
dc.description.funder | NASA | |
dc.description.funder | ESA | |
dc.description.funder | Space Telescope Science Institute | |
dc.description.funder | University of Southampton | |
dc.description.funder | Swiss National Science Foundation | |
dc.description.funder | FONDECYT | |
dc.description.funder | Ministry of Science and Higher Education of the Russian Federation | |
dc.fechaingreso.objetodigital | 2023-12-06 | |
dc.fuente.origen | SCOPUS | |
dc.identifier.doi | 10.1093/mnras/stad2989 | |
dc.identifier.eissn | 1365-2966 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.scopusid | SCOPUS_ID:85175622300 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/75479 | |
dc.identifier.wosid | WOS:001097539800001 | |
dc.information.autoruc | Instituto de Astrofísica ; Treister, Ezequiel ; 0000-0001-7568-6412 ; 1031846 | |
dc.information.autoruc | Instituto de Astrofísica ; Finlez, Carolina ; S/I ; 1161357 | |
dc.issue.numero | 3 | |
dc.language.iso | en | |
dc.nota.acceso | Contenido completo | |
dc.pagina.final | 4191 | |
dc.pagina.inicio | 4174 | |
dc.revista | Monthly Notices of the Royal Astronomical Society | |
dc.rights | acceso abierto | |
dc.subject | Galaxies: active | |
dc.subject | Galaxies: individual: NGC5972 | |
dc.subject | Galaxies: ISM | |
dc.subject | Galaxies: Seyfert | |
dc.subject | X-rays: galaxies | |
dc.subject.ddc | 520 | |
dc.subject.dewey | Astronomía | es_ES |
dc.subject.ods | 09 Industry, innovation and infrastructure | |
dc.subject.odspa | 09 Industria, innovación e infraestructura | |
dc.title | Signatures of feedback in the spectacular extended emission region of NGC 5972 | |
dc.type | artículo | |
dc.volumen | 526 | |
sipa.codpersvinculados | 1031846 | |
sipa.codpersvinculados | 1161357 | |
sipa.trazabilidad | SCOPUS;2023-11-19 |
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