Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

Autores: Sarangi, Arkaprabha; Zsíros, Szanna; Szalai, Tamás; Martinez, Laureano; Shahbandeh, Melissa; Fox, Ori D.; Van Dyk, Schuyler D.; Filippenko, Alexei V.; Bersten, Melina Cecilia; De Looze, Ilse; Ashall, Chris; Temim, Tea; Jencson, Jacob E.; Rest, Armin; Milisavljevic, Dan; Dessart, Luc; Dwek, Eli; Smith, Nathan; Tinyanont, Samaporn; Brink, Thomas G.; Zheng, WeiKang; Clayton, Geoffrey C.; Andrews, Jennifer
Año de publicación: 2025
Idioma: inglés
Tipo de recurso: artículo
Estado: versión publicada
Descripción: The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations a few years after explosion. Most theories of dust formation in SNe heavily rely only on SN 1987A. In the last two years, the James Webb Space Telescope (JWST) has enabled us to probe the dust evolution in decades-old SNe, such as SN 2004et, SN 2005ip, and SN 1980K. In this paper, we present two decades of dust evolution in SN 2005af, combining early-time infrared observations with the Spitzer Space Telescope and recent detections by the JWST. We have used a chemical kinetic model of dust synthesis in SN ejecta to develop a template of dust evolution in SN 2005af. Moreover, using this approach, for the first time, we have separately quantified the dust formed in the pre-explosion wind that survived after the explosion and the dust formed in the metal-rich SN ejecta post-explosion. We report that in SN 2005af, predominantly carbon-rich dust formed in the ejecta, with a total mass of at least 0.02 M⊙. In the circumstellar medium, the surviving oxygen-rich dust amounts to about (3─6) × 10−3 M⊙, yielding a total dust mass of at least 0.025 M⊙.
Fil: Sarangi, Arkaprabha. Indian Institute Of Astrophysics; India
Fil: Zsíros, Szanna. University Of Szeged; Hungría
Fil: Szalai, Tamás. University Of Szeged; Hungría
Fil: Martinez, Laureano. 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: Shahbandeh, Melissa. Space Telescope Science Institute; Estados Unidos
Fil: Fox, Ori D.. Space Telescope Science Institute; Estados Unidos
Fil: Van Dyk, Schuyler D.. California Institute of Technology; Estados Unidos
Fil: Filippenko, Alexei V.. University of California; Estados Unidos
Fil: Bersten, Melina Cecilia. 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: De Looze, Ilse. Sterrenkundig Observatorium; Bélgica
Fil: Ashall, Chris. University of Hawaii at Manoa; Estados Unidos
Fil: Temim, Tea. University of Princeton; Estados Unidos
Fil: Jencson, Jacob E.. California Institute of Technology; Estados Unidos
Fil: Rest, Armin. Space Telescope Science Institute; Estados Unidos
Fil: Milisavljevic, Dan. Purdue University; Estados Unidos
Fil: Dessart, Luc. Sorbonne University; Francia
Fil: Dwek, Eli. Observational Cosmology Lab; Estados Unidos
Fil: Smith, Nathan. Arizona State University; Estados Unidos
Fil: Tinyanont, Samaporn. National Astronomical Research Institute Of Thailand; Tailandia
Fil: Brink, Thomas G.. California State University; Estados Unidos
Fil: Zheng, WeiKang. California State University; Estados Unidos
Fil: Clayton, Geoffrey C.. State University of Louisiana; Estados Unidos
Fil: Andrews, Jennifer. Gemini Observatory; Estados Unidos
Materia: DUST FORMATION
CORE-COLLAPSE SUPERNOVAE
JAMES WEBB SPACE TELESCOPE
CIRCUMSTELLAR DUST
Nivel de accesibilidad: acceso abierto
Condiciones de uso: https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
Institución: Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador: oai:ri.conicet.gov.ar:11336/290879

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repository_id_str	3498
network_name_str	CONICET Digital (CONICET)
spelling	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical ModelingSarangi, ArkaprabhaZsíros, SzannaSzalai, TamásMartinez, LaureanoShahbandeh, MelissaFox, Ori D.Van Dyk, Schuyler D.Filippenko, Alexei V.Bersten, Melina CeciliaDe Looze, IlseAshall, ChrisTemim, TeaJencson, Jacob E.Rest, ArminMilisavljevic, DanDessart, LucDwek, EliSmith, NathanTinyanont, SamapornBrink, Thomas G.Zheng, WeiKangClayton, Geoffrey C.Andrews, JenniferDUST FORMATIONCORE-COLLAPSE SUPERNOVAEJAMES WEBB SPACE TELESCOPECIRCUMSTELLAR DUSThttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations a few years after explosion. Most theories of dust formation in SNe heavily rely only on SN 1987A. In the last two years, the James Webb Space Telescope (JWST) has enabled us to probe the dust evolution in decades-old SNe, such as SN 2004et, SN 2005ip, and SN 1980K. In this paper, we present two decades of dust evolution in SN 2005af, combining early-time infrared observations with the Spitzer Space Telescope and recent detections by the JWST. We have used a chemical kinetic model of dust synthesis in SN ejecta to develop a template of dust evolution in SN 2005af. Moreover, using this approach, for the first time, we have separately quantified the dust formed in the pre-explosion wind that survived after the explosion and the dust formed in the metal-rich SN ejecta post-explosion. We report that in SN 2005af, predominantly carbon-rich dust formed in the ejecta, with a total mass of at least 0.02 M⊙. In the circumstellar medium, the surviving oxygen-rich dust amounts to about (3─6) × 10−3 M⊙, yielding a total dust mass of at least 0.025 M⊙.Fil: Sarangi, Arkaprabha. Indian Institute Of Astrophysics; IndiaFil: Zsíros, Szanna. University Of Szeged; HungríaFil: Szalai, Tamás. University Of Szeged; HungríaFil: Martinez, Laureano. 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: Shahbandeh, Melissa. Space Telescope Science Institute; Estados UnidosFil: Fox, Ori D.. Space Telescope Science Institute; Estados UnidosFil: Van Dyk, Schuyler D.. California Institute of Technology; Estados UnidosFil: Filippenko, Alexei V.. University of California; Estados UnidosFil: Bersten, Melina Cecilia. 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: De Looze, Ilse. Sterrenkundig Observatorium; BélgicaFil: Ashall, Chris. University of Hawaii at Manoa; Estados UnidosFil: Temim, Tea. University of Princeton; Estados UnidosFil: Jencson, Jacob E.. California Institute of Technology; Estados UnidosFil: Rest, Armin. Space Telescope Science Institute; Estados UnidosFil: Milisavljevic, Dan. Purdue University; Estados UnidosFil: Dessart, Luc. Sorbonne University; FranciaFil: Dwek, Eli. Observational Cosmology Lab; Estados UnidosFil: Smith, Nathan. Arizona State University; Estados UnidosFil: Tinyanont, Samaporn. National Astronomical Research Institute Of Thailand; TailandiaFil: Brink, Thomas G.. California State University; Estados UnidosFil: Zheng, WeiKang. California State University; Estados UnidosFil: Clayton, Geoffrey C.. State University of Louisiana; Estados UnidosFil: Andrews, Jennifer. Gemini Observatory; Estados UnidosIOP Publishing2025-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/290879Sarangi, Arkaprabha; Zsíros, Szanna; Szalai, Tamás; Martinez, Laureano; Shahbandeh, Melissa; et al.; Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling; IOP Publishing; Astrophysical Journal; 993; 1; 10-2025; 1-150004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ae0645info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ae0645info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-08-25T14:53:59Zoai:ri.conicet.gov.ar:11336/290879instacron: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:34982026-08-25 14:53:59.597CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
title	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
spellingShingle	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling Sarangi, Arkaprabha DUST FORMATION CORE-COLLAPSE SUPERNOVAE JAMES WEBB SPACE TELESCOPE CIRCUMSTELLAR DUST
title_short	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
title_full	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
title_fullStr	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
title_full_unstemmed	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
title_sort	Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
dc.creator.none.fl_str_mv	Sarangi, Arkaprabha Zsíros, Szanna Szalai, Tamás Martinez, Laureano Shahbandeh, Melissa Fox, Ori D. Van Dyk, Schuyler D. Filippenko, Alexei V. Bersten, Melina Cecilia De Looze, Ilse Ashall, Chris Temim, Tea Jencson, Jacob E. Rest, Armin Milisavljevic, Dan Dessart, Luc Dwek, Eli Smith, Nathan Tinyanont, Samaporn Brink, Thomas G. Zheng, WeiKang Clayton, Geoffrey C. Andrews, Jennifer
author	Sarangi, Arkaprabha
author_facet	Sarangi, Arkaprabha Zsíros, Szanna Szalai, Tamás Martinez, Laureano Shahbandeh, Melissa Fox, Ori D. Van Dyk, Schuyler D. Filippenko, Alexei V. Bersten, Melina Cecilia De Looze, Ilse Ashall, Chris Temim, Tea Jencson, Jacob E. Rest, Armin Milisavljevic, Dan Dessart, Luc Dwek, Eli Smith, Nathan Tinyanont, Samaporn Brink, Thomas G. Zheng, WeiKang Clayton, Geoffrey C. Andrews, Jennifer
author_role	author
author2	Zsíros, Szanna Szalai, Tamás Martinez, Laureano Shahbandeh, Melissa Fox, Ori D. Van Dyk, Schuyler D. Filippenko, Alexei V. Bersten, Melina Cecilia De Looze, Ilse Ashall, Chris Temim, Tea Jencson, Jacob E. Rest, Armin Milisavljevic, Dan Dessart, Luc Dwek, Eli Smith, Nathan Tinyanont, Samaporn Brink, Thomas G. Zheng, WeiKang Clayton, Geoffrey C. Andrews, Jennifer
author2_role	author author author author author author author author author author author author author author author author author author author author author author
dc.subject.none.fl_str_mv	DUST FORMATION CORE-COLLAPSE SUPERNOVAE JAMES WEBB SPACE TELESCOPE CIRCUMSTELLAR DUST
topic	DUST FORMATION CORE-COLLAPSE SUPERNOVAE JAMES WEBB SPACE TELESCOPE CIRCUMSTELLAR DUST
purl_subject.fl_str_mv	https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv	The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations a few years after explosion. Most theories of dust formation in SNe heavily rely only on SN 1987A. In the last two years, the James Webb Space Telescope (JWST) has enabled us to probe the dust evolution in decades-old SNe, such as SN 2004et, SN 2005ip, and SN 1980K. In this paper, we present two decades of dust evolution in SN 2005af, combining early-time infrared observations with the Spitzer Space Telescope and recent detections by the JWST. We have used a chemical kinetic model of dust synthesis in SN ejecta to develop a template of dust evolution in SN 2005af. Moreover, using this approach, for the first time, we have separately quantified the dust formed in the pre-explosion wind that survived after the explosion and the dust formed in the metal-rich SN ejecta post-explosion. We report that in SN 2005af, predominantly carbon-rich dust formed in the ejecta, with a total mass of at least 0.02 M⊙. In the circumstellar medium, the surviving oxygen-rich dust amounts to about (3─6) × 10−3 M⊙, yielding a total dust mass of at least 0.025 M⊙. Fil: Sarangi, Arkaprabha. Indian Institute Of Astrophysics; India Fil: Zsíros, Szanna. University Of Szeged; Hungría Fil: Szalai, Tamás. University Of Szeged; Hungría Fil: Martinez, Laureano. 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: Shahbandeh, Melissa. Space Telescope Science Institute; Estados Unidos Fil: Fox, Ori D.. Space Telescope Science Institute; Estados Unidos Fil: Van Dyk, Schuyler D.. California Institute of Technology; Estados Unidos Fil: Filippenko, Alexei V.. University of California; Estados Unidos Fil: Bersten, Melina Cecilia. 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: De Looze, Ilse. Sterrenkundig Observatorium; Bélgica Fil: Ashall, Chris. University of Hawaii at Manoa; Estados Unidos Fil: Temim, Tea. University of Princeton; Estados Unidos Fil: Jencson, Jacob E.. California Institute of Technology; Estados Unidos Fil: Rest, Armin. Space Telescope Science Institute; Estados Unidos Fil: Milisavljevic, Dan. Purdue University; Estados Unidos Fil: Dessart, Luc. Sorbonne University; Francia Fil: Dwek, Eli. Observational Cosmology Lab; Estados Unidos Fil: Smith, Nathan. Arizona State University; Estados Unidos Fil: Tinyanont, Samaporn. National Astronomical Research Institute Of Thailand; Tailandia Fil: Brink, Thomas G.. California State University; Estados Unidos Fil: Zheng, WeiKang. California State University; Estados Unidos Fil: Clayton, Geoffrey C.. State University of Louisiana; Estados Unidos Fil: Andrews, Jennifer. Gemini Observatory; Estados Unidos
description	The evolution of dust in core-collapse supernovae (SNe), in general, is poorly constrained owing to a lack of infrared observations a few years after explosion. Most theories of dust formation in SNe heavily rely only on SN 1987A. In the last two years, the James Webb Space Telescope (JWST) has enabled us to probe the dust evolution in decades-old SNe, such as SN 2004et, SN 2005ip, and SN 1980K. In this paper, we present two decades of dust evolution in SN 2005af, combining early-time infrared observations with the Spitzer Space Telescope and recent detections by the JWST. We have used a chemical kinetic model of dust synthesis in SN ejecta to develop a template of dust evolution in SN 2005af. Moreover, using this approach, for the first time, we have separately quantified the dust formed in the pre-explosion wind that survived after the explosion and the dust formed in the metal-rich SN ejecta post-explosion. We report that in SN 2005af, predominantly carbon-rich dust formed in the ejecta, with a total mass of at least 0.02 M⊙. In the circumstellar medium, the surviving oxygen-rich dust amounts to about (3─6) × 10−3 M⊙, yielding a total dust mass of at least 0.025 M⊙.
publishDate	2025
dc.date.none.fl_str_mv	2025-10
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/11336/290879 Sarangi, Arkaprabha; Zsíros, Szanna; Szalai, Tamás; Martinez, Laureano; Shahbandeh, Melissa; et al.; Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling; IOP Publishing; Astrophysical Journal; 993; 1; 10-2025; 1-15 0004-637X CONICET Digital CONICET
url	http://hdl.handle.net/11336/290879
identifier_str_mv	Sarangi, Arkaprabha; Zsíros, Szanna; Szalai, Tamás; Martinez, Laureano; Shahbandeh, Melissa; et al.; Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling; IOP Publishing; Astrophysical Journal; 993; 1; 10-2025; 1-15 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/ae0645 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ae0645
dc.rights.none.fl_str_mv	info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/
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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)
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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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Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling

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