Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946

Autores
Lara López, M. A.; Pilyugin, L. S.; Zaragoza Cardiel, J.; Zinchenko, I.A.; López Cruz, Omar; O'sullivan, S. P.; de Rossi, Maria Emilia; Dib, S.; Garduño, L. E.; Rosado, M.; Sánchez Cruces, M.; Valerdi, M.
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Context. NGC 6946, also known as the-Fireworks Galaxy, is an unusual galaxy that hosts a total of 225 supernova remnant (SNR) candidates, including 147 optically identified with high [SII]/Hα line ratios. In addition, this galaxy shows prominent HI holes, which have been analyzed in previous studies. Indeed, the connection between SNRs and HI holes along with their physical implications in the surrounding gas are worthy of attention. Aims. This paper explores the connection between the SNRs and the HI holes, including an analysis of their physical link to observational optical properties inside and around the rims of the holes, using new integral field unit (IFU) data from the Metal-THINGS survey. Methods. We present an analysis combining previously identified HI holes, SNR candidates, and new integral field unit (IFU) data from Metal-THINGS of the spiral galaxy NGC 6946. We analyzed the distributions of the oxygen abundance, star formation rate surface density, extinction, ionization, and diffuse ionized gas, as well as the Baldwin-Phillips-Terlevich classification throughout the galaxy. Results. By analyzing the optical properties of the 121 previously identify HI holes in NGC 6946 in detail, we find that the SNRs are concentrated at the rims of the HI holes. Furthermore, our IFU data show that the star formation rate and extinction are enhanced at the rims of the holes. To a lesser degree, the oxygen abundance and ionization parameter show hints of enhancement on the rims of the holes. Altogether, this provides evidence of induced star formation taking place at the rims of the holes, whose origin can be explained by the expansion of superbubbles created by multiple supernova explosions in large stellar clusters dozens of Myr ago.
Fil: Lara López, M. A.. Universidad Complutense de Madrid; España
Fil: Pilyugin, L. S.. National Academy of Sciences of Ukraine; Ucrania. Vilnius University; Lituania
Fil: Zaragoza Cardiel, J.. Instituto Nacional de Astrofisica Optica y Electronica; México. Consejo Nacional de Ciencia y Tecnología; México
Fil: Zinchenko, I.A.. Ludwig Maximilians Universitat; Alemania. National Academy of Sciences of Ukraine; Ucrania
Fil: López Cruz, Omar. Instituto Nacional de Astrofisica Optica y Electronica; México
Fil: O'sullivan, S. P.. Dublin City University; Irlanda
Fil: de Rossi, Maria Emilia. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Dib, S.. Max Planck Institute For Astronomy; Alemania
Fil: Garduño, L. E.. Instituto Nacional de Astrofisica Optica y Electronica; México
Fil: Rosado, M.. Universidad Nacional Autónoma de México; México
Fil: Sánchez Cruces, M.. Universidad Nacional Autónoma de México; México
Fil: Valerdi, M.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México
Materia
GALAXIES: ABUNDANCES
GALAXIES: ISM
GALAXIES: SPIRAL
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:11336/219272
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/219272
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946Lara López, M. A.Pilyugin, L. S.Zaragoza Cardiel, J.Zinchenko, I.A.López Cruz, OmarO'sullivan, S. P.de Rossi, Maria EmiliaDib, S.Garduño, L. E.Rosado, M.Sánchez Cruces, M.Valerdi, M.GALAXIES: ABUNDANCESGALAXIES: ISMGALAXIES: SPIRALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. NGC 6946, also known as the-Fireworks Galaxy, is an unusual galaxy that hosts a total of 225 supernova remnant (SNR) candidates, including 147 optically identified with high [SII]/Hα line ratios. In addition, this galaxy shows prominent HI holes, which have been analyzed in previous studies. Indeed, the connection between SNRs and HI holes along with their physical implications in the surrounding gas are worthy of attention. Aims. This paper explores the connection between the SNRs and the HI holes, including an analysis of their physical link to observational optical properties inside and around the rims of the holes, using new integral field unit (IFU) data from the Metal-THINGS survey. Methods. We present an analysis combining previously identified HI holes, SNR candidates, and new integral field unit (IFU) data from Metal-THINGS of the spiral galaxy NGC 6946. We analyzed the distributions of the oxygen abundance, star formation rate surface density, extinction, ionization, and diffuse ionized gas, as well as the Baldwin-Phillips-Terlevich classification throughout the galaxy. Results. By analyzing the optical properties of the 121 previously identify HI holes in NGC 6946 in detail, we find that the SNRs are concentrated at the rims of the HI holes. Furthermore, our IFU data show that the star formation rate and extinction are enhanced at the rims of the holes. To a lesser degree, the oxygen abundance and ionization parameter show hints of enhancement on the rims of the holes. Altogether, this provides evidence of induced star formation taking place at the rims of the holes, whose origin can be explained by the expansion of superbubbles created by multiple supernova explosions in large stellar clusters dozens of Myr ago.Fil: Lara López, M. A.. Universidad Complutense de Madrid; EspañaFil: Pilyugin, L. S.. National Academy of Sciences of Ukraine; Ucrania. Vilnius University; LituaniaFil: Zaragoza Cardiel, J.. Instituto Nacional de Astrofisica Optica y Electronica; México. Consejo Nacional de Ciencia y Tecnología; MéxicoFil: Zinchenko, I.A.. Ludwig Maximilians Universitat; Alemania. National Academy of Sciences of Ukraine; UcraniaFil: López Cruz, Omar. Instituto Nacional de Astrofisica Optica y Electronica; MéxicoFil: O'sullivan, S. P.. Dublin City University; IrlandaFil: de Rossi, Maria Emilia. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Dib, S.. Max Planck Institute For Astronomy; AlemaniaFil: Garduño, L. E.. Instituto Nacional de Astrofisica Optica y Electronica; MéxicoFil: Rosado, M.. Universidad Nacional Autónoma de México; MéxicoFil: Sánchez Cruces, M.. Universidad Nacional Autónoma de México; MéxicoFil: Valerdi, M.. Instituto Nacional de Astrofísica, Óptica y Electrónica; MéxicoEDP Sciences2023-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/219272Lara López, M. A.; Pilyugin, L. S.; Zaragoza Cardiel, J.; Zinchenko, I.A.; López Cruz, Omar; et al.; Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946; EDP Sciences; Astronomy and Astrophysics; 669; A25; 1-2023; 1-110004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202245068info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2023/01/aa45068-22/aa45068-22.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:06:39Zoai:ri.conicet.gov.ar:11336/219272instacron: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:34982025-10-22 11:06:39.721CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
title Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
spellingShingle Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
Lara López, M. A.
GALAXIES: ABUNDANCES
GALAXIES: ISM
GALAXIES: SPIRAL
title_short Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
title_full Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
title_fullStr Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
title_full_unstemmed Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
title_sort Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946
dc.creator.none.fl_str_mv Lara López, M. A.
Pilyugin, L. S.
Zaragoza Cardiel, J.
Zinchenko, I.A.
López Cruz, Omar
O'sullivan, S. P.
de Rossi, Maria Emilia
Dib, S.
Garduño, L. E.
Rosado, M.
Sánchez Cruces, M.
Valerdi, M.
author Lara López, M. A.
author_facet Lara López, M. A.
Pilyugin, L. S.
Zaragoza Cardiel, J.
Zinchenko, I.A.
López Cruz, Omar
O'sullivan, S. P.
de Rossi, Maria Emilia
Dib, S.
Garduño, L. E.
Rosado, M.
Sánchez Cruces, M.
Valerdi, M.
author_role author
author2 Pilyugin, L. S.
Zaragoza Cardiel, J.
Zinchenko, I.A.
López Cruz, Omar
O'sullivan, S. P.
de Rossi, Maria Emilia
Dib, S.
Garduño, L. E.
Rosado, M.
Sánchez Cruces, M.
Valerdi, M.
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: ABUNDANCES
GALAXIES: ISM
GALAXIES: SPIRAL
topic GALAXIES: ABUNDANCES
GALAXIES: ISM
GALAXIES: SPIRAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Context. NGC 6946, also known as the-Fireworks Galaxy, is an unusual galaxy that hosts a total of 225 supernova remnant (SNR) candidates, including 147 optically identified with high [SII]/Hα line ratios. In addition, this galaxy shows prominent HI holes, which have been analyzed in previous studies. Indeed, the connection between SNRs and HI holes along with their physical implications in the surrounding gas are worthy of attention. Aims. This paper explores the connection between the SNRs and the HI holes, including an analysis of their physical link to observational optical properties inside and around the rims of the holes, using new integral field unit (IFU) data from the Metal-THINGS survey. Methods. We present an analysis combining previously identified HI holes, SNR candidates, and new integral field unit (IFU) data from Metal-THINGS of the spiral galaxy NGC 6946. We analyzed the distributions of the oxygen abundance, star formation rate surface density, extinction, ionization, and diffuse ionized gas, as well as the Baldwin-Phillips-Terlevich classification throughout the galaxy. Results. By analyzing the optical properties of the 121 previously identify HI holes in NGC 6946 in detail, we find that the SNRs are concentrated at the rims of the HI holes. Furthermore, our IFU data show that the star formation rate and extinction are enhanced at the rims of the holes. To a lesser degree, the oxygen abundance and ionization parameter show hints of enhancement on the rims of the holes. Altogether, this provides evidence of induced star formation taking place at the rims of the holes, whose origin can be explained by the expansion of superbubbles created by multiple supernova explosions in large stellar clusters dozens of Myr ago.
Fil: Lara López, M. A.. Universidad Complutense de Madrid; España
Fil: Pilyugin, L. S.. National Academy of Sciences of Ukraine; Ucrania. Vilnius University; Lituania
Fil: Zaragoza Cardiel, J.. Instituto Nacional de Astrofisica Optica y Electronica; México. Consejo Nacional de Ciencia y Tecnología; México
Fil: Zinchenko, I.A.. Ludwig Maximilians Universitat; Alemania. National Academy of Sciences of Ukraine; Ucrania
Fil: López Cruz, Omar. Instituto Nacional de Astrofisica Optica y Electronica; México
Fil: O'sullivan, S. P.. Dublin City University; Irlanda
Fil: de Rossi, Maria Emilia. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Dib, S.. Max Planck Institute For Astronomy; Alemania
Fil: Garduño, L. E.. Instituto Nacional de Astrofisica Optica y Electronica; México
Fil: Rosado, M.. Universidad Nacional Autónoma de México; México
Fil: Sánchez Cruces, M.. Universidad Nacional Autónoma de México; México
Fil: Valerdi, M.. Instituto Nacional de Astrofísica, Óptica y Electrónica; México
description Context. NGC 6946, also known as the-Fireworks Galaxy, is an unusual galaxy that hosts a total of 225 supernova remnant (SNR) candidates, including 147 optically identified with high [SII]/Hα line ratios. In addition, this galaxy shows prominent HI holes, which have been analyzed in previous studies. Indeed, the connection between SNRs and HI holes along with their physical implications in the surrounding gas are worthy of attention. Aims. This paper explores the connection between the SNRs and the HI holes, including an analysis of their physical link to observational optical properties inside and around the rims of the holes, using new integral field unit (IFU) data from the Metal-THINGS survey. Methods. We present an analysis combining previously identified HI holes, SNR candidates, and new integral field unit (IFU) data from Metal-THINGS of the spiral galaxy NGC 6946. We analyzed the distributions of the oxygen abundance, star formation rate surface density, extinction, ionization, and diffuse ionized gas, as well as the Baldwin-Phillips-Terlevich classification throughout the galaxy. Results. By analyzing the optical properties of the 121 previously identify HI holes in NGC 6946 in detail, we find that the SNRs are concentrated at the rims of the HI holes. Furthermore, our IFU data show that the star formation rate and extinction are enhanced at the rims of the holes. To a lesser degree, the oxygen abundance and ionization parameter show hints of enhancement on the rims of the holes. Altogether, this provides evidence of induced star formation taking place at the rims of the holes, whose origin can be explained by the expansion of superbubbles created by multiple supernova explosions in large stellar clusters dozens of Myr ago.
publishDate 2023
dc.date.none.fl_str_mv 2023-01
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/11336/219272
Lara López, M. A.; Pilyugin, L. S.; Zaragoza Cardiel, J.; Zinchenko, I.A.; López Cruz, Omar; et al.; Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946; EDP Sciences; Astronomy and Astrophysics; 669; A25; 1-2023; 1-11
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/219272
identifier_str_mv Lara López, M. A.; Pilyugin, L. S.; Zaragoza Cardiel, J.; Zinchenko, I.A.; López Cruz, Omar; et al.; Metal-THINGS: Association and optical characterization of supernova remnants with H I holes in NGC 6946; EDP Sciences; Astronomy and Astrophysics; 669; A25; 1-2023; 1-11
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202245068
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2023/01/aa45068-22/aa45068-22.html
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 EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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 13.229304

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