Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58

Autores
Ogle, Patrick M.; López, Iván Emanuel; Reynaldi, María Victoria; Togi, Aditya; Rich, R. Michael; Román, Javier; Caceres, Osmin; Li, Zhuofu; Donnelly, Grant; Smith, J. D. T.; Appleton, Philip N.; Lanz, Lauranne
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1–0 S(1) emission line, Atacama Large Millimeter/submillimeter Array CO 2–1, and Hubble Space Telescope multiband imagery indicate that much of the molecular gas is shocked in situ, corresponding to lanes of dusty molecular gas that spiral toward the galactic nucleus. The CO 2–1 and ionized gas kinematics are highly disturbed, with velocity dispersion up to 300 km s−1. Dissipation of the associated kinetic energy and turbulence, likely injected into the interstellar medium by radio-jet-driven outflows, may power the observed molecular and ionized gas emission from the inner disk. The polycyclic aromatic hydrocarbon (PAH) fraction and composition in the inner disk appear to be normal, in spite of the jet and AGN activity. The PAH ratios are consistent with excitation by the interstellar radiation field from old stars in the bulge, with no contribution from star formation. The phenomenon of jet-shocked H2 may substantially reduce star formation and help to regulate the stellar mass of the inner disk and supermassive black hole in this otherwise normal spiral galaxy. Similarly strong H2 emission is found at the centers of several nearby spiral and lenticular galaxies with massive bulges and radio-loud AGNs.
Fil: Ogle, Patrick M.. Space Telescope Science Institute; Estados Unidos
Fil: López, Iván Emanuel. Space Telescope Science Institute; Estados Unidos
Fil: Reynaldi, María Victoria. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Togi, Aditya. University Of Texas. Departament Of Physics; Estados Unidos
Fil: Rich, R. Michael. University of California; Estados Unidos
Fil: Román, Javier. University Of Groningen. Departament Of Astronomy. Kapteyn Astronómical Institute; Países Bajos
Fil: Caceres, Osmin. University of California; Estados Unidos
Fil: Li, Zhuofu. University of California; Estados Unidos
Fil: Donnelly, Grant. Ritter Astrophysical Research Center; Estados Unidos
Fil: Smith, J. D. T.. Ritter Astrophysical Research Center; Estados Unidos
Fil: Appleton, Philip N.. California Institute of Technology; Estados Unidos
Fil: Lanz, Lauranne. The College of New Yersey; Estados Unidos
Materia
ACTIVE GALAXIES
RADIO JETS
SHOCKS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/236854
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58Ogle, Patrick M.López, Iván EmanuelReynaldi, María VictoriaTogi, AdityaRich, R. MichaelRomán, JavierCaceres, OsminLi, ZhuofuDonnelly, GrantSmith, J. D. T.Appleton, Philip N.Lanz, LauranneACTIVE GALAXIESRADIO JETSSHOCKShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1–0 S(1) emission line, Atacama Large Millimeter/submillimeter Array CO 2–1, and Hubble Space Telescope multiband imagery indicate that much of the molecular gas is shocked in situ, corresponding to lanes of dusty molecular gas that spiral toward the galactic nucleus. The CO 2–1 and ionized gas kinematics are highly disturbed, with velocity dispersion up to 300 km s−1. Dissipation of the associated kinetic energy and turbulence, likely injected into the interstellar medium by radio-jet-driven outflows, may power the observed molecular and ionized gas emission from the inner disk. The polycyclic aromatic hydrocarbon (PAH) fraction and composition in the inner disk appear to be normal, in spite of the jet and AGN activity. The PAH ratios are consistent with excitation by the interstellar radiation field from old stars in the bulge, with no contribution from star formation. The phenomenon of jet-shocked H2 may substantially reduce star formation and help to regulate the stellar mass of the inner disk and supermassive black hole in this otherwise normal spiral galaxy. Similarly strong H2 emission is found at the centers of several nearby spiral and lenticular galaxies with massive bulges and radio-loud AGNs.Fil: Ogle, Patrick M.. Space Telescope Science Institute; Estados UnidosFil: López, Iván Emanuel. Space Telescope Science Institute; Estados UnidosFil: Reynaldi, María Victoria. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Togi, Aditya. University Of Texas. Departament Of Physics; Estados UnidosFil: Rich, R. Michael. University of California; Estados UnidosFil: Román, Javier. University Of Groningen. Departament Of Astronomy. Kapteyn Astronómical Institute; Países BajosFil: Caceres, Osmin. University of California; Estados UnidosFil: Li, Zhuofu. University of California; Estados UnidosFil: Donnelly, Grant. Ritter Astrophysical Research Center; Estados UnidosFil: Smith, J. D. T.. Ritter Astrophysical Research Center; Estados UnidosFil: Appleton, Philip N.. California Institute of Technology; Estados UnidosFil: Lanz, Lauranne. The College of New Yersey; Estados UnidosIOP Publishing2024-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/236854Ogle, Patrick M.; López, Iván Emanuel; Reynaldi, María Victoria; Togi, Aditya; Rich, R. Michael; et al.; Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58; IOP Publishing; Astrophysical Journal; 962; 2; 2-2024; 1-160004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad1242info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad1242info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:59:16Zoai:ri.conicet.gov.ar:11336/236854instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:59:16.667CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
title Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
spellingShingle Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
Ogle, Patrick M.
ACTIVE GALAXIES
RADIO JETS
SHOCKS
title_short Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
title_full Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
title_fullStr Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
title_full_unstemmed Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
title_sort Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58
dc.creator.none.fl_str_mv Ogle, Patrick M.
López, Iván Emanuel
Reynaldi, María Victoria
Togi, Aditya
Rich, R. Michael
Román, Javier
Caceres, Osmin
Li, Zhuofu
Donnelly, Grant
Smith, J. D. T.
Appleton, Philip N.
Lanz, Lauranne
author Ogle, Patrick M.
author_facet Ogle, Patrick M.
López, Iván Emanuel
Reynaldi, María Victoria
Togi, Aditya
Rich, R. Michael
Román, Javier
Caceres, Osmin
Li, Zhuofu
Donnelly, Grant
Smith, J. D. T.
Appleton, Philip N.
Lanz, Lauranne
author_role author
author2 López, Iván Emanuel
Reynaldi, María Victoria
Togi, Aditya
Rich, R. Michael
Román, Javier
Caceres, Osmin
Li, Zhuofu
Donnelly, Grant
Smith, J. D. T.
Appleton, Philip N.
Lanz, Lauranne
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv ACTIVE GALAXIES
RADIO JETS
SHOCKS
topic ACTIVE GALAXIES
RADIO JETS
SHOCKS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1–0 S(1) emission line, Atacama Large Millimeter/submillimeter Array CO 2–1, and Hubble Space Telescope multiband imagery indicate that much of the molecular gas is shocked in situ, corresponding to lanes of dusty molecular gas that spiral toward the galactic nucleus. The CO 2–1 and ionized gas kinematics are highly disturbed, with velocity dispersion up to 300 km s−1. Dissipation of the associated kinetic energy and turbulence, likely injected into the interstellar medium by radio-jet-driven outflows, may power the observed molecular and ionized gas emission from the inner disk. The polycyclic aromatic hydrocarbon (PAH) fraction and composition in the inner disk appear to be normal, in spite of the jet and AGN activity. The PAH ratios are consistent with excitation by the interstellar radiation field from old stars in the bulge, with no contribution from star formation. The phenomenon of jet-shocked H2 may substantially reduce star formation and help to regulate the stellar mass of the inner disk and supermassive black hole in this otherwise normal spiral galaxy. Similarly strong H2 emission is found at the centers of several nearby spiral and lenticular galaxies with massive bulges and radio-loud AGNs.
Fil: Ogle, Patrick M.. Space Telescope Science Institute; Estados Unidos
Fil: López, Iván Emanuel. Space Telescope Science Institute; Estados Unidos
Fil: Reynaldi, María Victoria. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Togi, Aditya. University Of Texas. Departament Of Physics; Estados Unidos
Fil: Rich, R. Michael. University of California; Estados Unidos
Fil: Román, Javier. University Of Groningen. Departament Of Astronomy. Kapteyn Astronómical Institute; Países Bajos
Fil: Caceres, Osmin. University of California; Estados Unidos
Fil: Li, Zhuofu. University of California; Estados Unidos
Fil: Donnelly, Grant. Ritter Astrophysical Research Center; Estados Unidos
Fil: Smith, J. D. T.. Ritter Astrophysical Research Center; Estados Unidos
Fil: Appleton, Philip N.. California Institute of Technology; Estados Unidos
Fil: Lanz, Lauranne. The College of New Yersey; Estados Unidos
description Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1–0 S(1) emission line, Atacama Large Millimeter/submillimeter Array CO 2–1, and Hubble Space Telescope multiband imagery indicate that much of the molecular gas is shocked in situ, corresponding to lanes of dusty molecular gas that spiral toward the galactic nucleus. The CO 2–1 and ionized gas kinematics are highly disturbed, with velocity dispersion up to 300 km s−1. Dissipation of the associated kinetic energy and turbulence, likely injected into the interstellar medium by radio-jet-driven outflows, may power the observed molecular and ionized gas emission from the inner disk. The polycyclic aromatic hydrocarbon (PAH) fraction and composition in the inner disk appear to be normal, in spite of the jet and AGN activity. The PAH ratios are consistent with excitation by the interstellar radiation field from old stars in the bulge, with no contribution from star formation. The phenomenon of jet-shocked H2 may substantially reduce star formation and help to regulate the stellar mass of the inner disk and supermassive black hole in this otherwise normal spiral galaxy. Similarly strong H2 emission is found at the centers of several nearby spiral and lenticular galaxies with massive bulges and radio-loud AGNs.
publishDate 2024
dc.date.none.fl_str_mv 2024-02
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/236854
Ogle, Patrick M.; López, Iván Emanuel; Reynaldi, María Victoria; Togi, Aditya; Rich, R. Michael; et al.; Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58; IOP Publishing; Astrophysical Journal; 962; 2; 2-2024; 1-16
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/236854
identifier_str_mv Ogle, Patrick M.; López, Iván Emanuel; Reynaldi, María Victoria; Togi, Aditya; Rich, R. Michael; et al.; Radio jet feedback on the inner disk of Virgo Spiral Galaxy Messier 58; IOP Publishing; Astrophysical Journal; 962; 2; 2-2024; 1-16
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad1242
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad1242
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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