Signatures of feedback in the spectacular extended emission region of NGC 5972

dc.catalogadordfo
dc.contributor.authorHarvey, Thomas
dc.contributor.authorMaksym, W. Peter
dc.contributor.authorKeel, William
dc.contributor.authorKoss, Michael
dc.contributor.authorBennert, Vardha N.
dc.contributor.authorChojnowski, S. Drew
dc.contributor.authorTreister, Ezequiel
dc.contributor.authorFinlez, Carolina
dc.contributor.authorLintott, Chris J.
dc.contributor.authorMoiseev, Alexei
dc.contributor.authorSimmons, Brooke D.
dc.contributor.authorSartori, Lia F.
dc.contributor.authorUrry, Megan
dc.date.accessioned2023-12-06T20:47:12Z
dc.date.available2023-12-06T20:47:12Z
dc.date.issued2023
dc.description.abstractWe 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.funderCenter for Astrophysics
dc.description.funderChandra Source Catalog
dc.description.funderChandra X-ray Center
dc.description.funderNational Science Foundation
dc.description.funderNASA
dc.description.funderESA
dc.description.funderSpace Telescope Science Institute
dc.description.funderUniversity of Southampton
dc.description.funderSwiss National Science Foundation
dc.description.funderFONDECYT
dc.description.funderMinistry of Science and Higher Education of the Russian Federation
dc.fechaingreso.objetodigital2023-12-06
dc.fuente.origenSCOPUS
dc.identifier.doi10.1093/mnras/stad2989
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.scopusidSCOPUS_ID:85175622300
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/75479
dc.identifier.wosidWOS:001097539800001
dc.information.autorucInstituto de Astrofísica ; Treister, Ezequiel ; 0000-0001-7568-6412 ; 1031846
dc.information.autorucInstituto de Astrofísica ; Finlez, Carolina ; S/I ; 1161357
dc.issue.numero3
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final4191
dc.pagina.inicio4174
dc.revistaMonthly Notices of the Royal Astronomical Society
dc.rightsacceso abierto
dc.subjectGalaxies: active
dc.subjectGalaxies: individual: NGC5972
dc.subjectGalaxies: ISM
dc.subjectGalaxies: Seyfert
dc.subjectX-rays: galaxies
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.ods09 Industry, innovation and infrastructure
dc.subject.odspa09 Industria, innovación e infraestructura
dc.titleSignatures of feedback in the spectacular extended emission region of NGC 5972
dc.typeartículo
dc.volumen526
sipa.codpersvinculados1031846
sipa.codpersvinculados1161357
sipa.trazabilidadSCOPUS;2023-11-19
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