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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/219272
Ver los metadatos del registro completo
id |
CONICETDig_60ab14aeae5d7f1c06aaf58db4bcc4a2 |
---|---|
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 Técnicas2025-09-29T09:38:24Zoai: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:34982025-09-29 09:38:24.813CONICET 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 |
_version_ |
1844613213649371136 |
score |
13.070432 |