Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star

Autores
Fang, Qiliang; Moriya, Takashi J.; Ferrari, Lucía; Maeda, Keiichi; Folatelli, Gaston; Ertini, Keila Yael; Kuncarayakti, Hanindyo; Andrews, Jennifer E.; Matsumoto, Tatsuya
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
SN 2023ixf is one of the most well-observed core-collapse supernovae in recent decades, yet there is inconsistencyin the inferred zero-age main-sequence (ZAMS) mass MZAMS of its progenitor. Direct observations of the pre-supernova (SN) red supergiant (RSG) estimate MZAMS spanning widely from 11 to 18 Me. Additional constraints,including the host environment and the pulsation of its progenitor RSG, suggest a massive progenitor withMZAMS > 17 Me. However, the analysis of the SN properties, from light-curve modeling to late-phasespectroscopy, favors a relatively low-mass scenario (MZAMS < 15 Me). In this work, we conduct a systematicanalysis of SN 2023ixf, from the RSG progenitor, plateau phase light curve to late-phase spectroscopy. UsingMESA+STELLA to simulate the RSG progenitor and their explosions, we find that a range of the RSG modelshaving MZAMS that vary from 12 to 17.5 Me can reproduce its multiband light curves if the hydrogen-rich envelopemass and the explosion energy are allowed to vary. Using late-phase spectroscopy as an independent measurement,the oxygen line [O I] indicates an intermediate-massive progenitor (MZAMS ∼ 16.0 Me). By incorporating thevelocity structure derived from the light-curve modeling into an axisymmetric model, we generated [O I] lineprofiles that are consistent with the [O I] line observed in late-phase spectroscopy of SN 2023ixf. Bringing theseanalyses together, we conclude that SN 2023ixf is the aspherical explosion of an intermediate-massive star(MZAMS = 15–16 Me), with the hydrogen envelope being stripped to 4–5 Me prior to its explosion.
Fil: Fang, Qiliang. National Institutes of Natural Sciences; Japón
Fil: Moriya, Takashi J.. National Institutes of Natural Sciences; Japón
Fil: Ferrari, Lucía. 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: Maeda, Keiichi. National Institutes of Natural Sciences; Japón
Fil: Folatelli, Gaston. 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: Ertini, Keila Yael. 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: Kuncarayakti, Hanindyo. University of Turku; Finlandia
Fil: Andrews, Jennifer E.. No especifíca;
Fil: Matsumoto, Tatsuya. Kyoto University; Japón
Materia
Supernovae:general
Supernovae:Individual:SN2023ixf
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:11336/266245
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive StarFang, QiliangMoriya, Takashi J.Ferrari, LucíaMaeda, KeiichiFolatelli, GastonErtini, Keila YaelKuncarayakti, HanindyoAndrews, Jennifer E.Matsumoto, TatsuyaSupernovae:generalSupernovae:Individual:SN2023ixfhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1SN 2023ixf is one of the most well-observed core-collapse supernovae in recent decades, yet there is inconsistencyin the inferred zero-age main-sequence (ZAMS) mass MZAMS of its progenitor. Direct observations of the pre-supernova (SN) red supergiant (RSG) estimate MZAMS spanning widely from 11 to 18 Me. Additional constraints,including the host environment and the pulsation of its progenitor RSG, suggest a massive progenitor withMZAMS > 17 Me. However, the analysis of the SN properties, from light-curve modeling to late-phasespectroscopy, favors a relatively low-mass scenario (MZAMS < 15 Me). In this work, we conduct a systematicanalysis of SN 2023ixf, from the RSG progenitor, plateau phase light curve to late-phase spectroscopy. UsingMESA+STELLA to simulate the RSG progenitor and their explosions, we find that a range of the RSG modelshaving MZAMS that vary from 12 to 17.5 Me can reproduce its multiband light curves if the hydrogen-rich envelopemass and the explosion energy are allowed to vary. Using late-phase spectroscopy as an independent measurement,the oxygen line [O I] indicates an intermediate-massive progenitor (MZAMS ∼ 16.0 Me). By incorporating thevelocity structure derived from the light-curve modeling into an axisymmetric model, we generated [O I] lineprofiles that are consistent with the [O I] line observed in late-phase spectroscopy of SN 2023ixf. Bringing theseanalyses together, we conclude that SN 2023ixf is the aspherical explosion of an intermediate-massive star(MZAMS = 15–16 Me), with the hydrogen envelope being stripped to 4–5 Me prior to its explosion.Fil: Fang, Qiliang. National Institutes of Natural Sciences; JapónFil: Moriya, Takashi J.. National Institutes of Natural Sciences; JapónFil: Ferrari, Lucía. 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: Maeda, Keiichi. National Institutes of Natural Sciences; JapónFil: Folatelli, Gaston. 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: Ertini, Keila Yael. 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: Kuncarayakti, Hanindyo. University of Turku; FinlandiaFil: Andrews, Jennifer E.. No especifíca;Fil: Matsumoto, Tatsuya. Kyoto University; JapónIOP Publishing2024-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/266245Fang, Qiliang; Moriya, Takashi J.; Ferrari, Lucía; Maeda, Keiichi; Folatelli, Gaston; et al.; Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star; IOP Publishing; Astrophysical Journal; 978; 1; 12-2024; 1-100004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad8d5ainfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad8d5ainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:31:39Zoai:ri.conicet.gov.ar:11336/266245instacron: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 10:31:39.498CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
title Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
spellingShingle Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
Fang, Qiliang
Supernovae:general
Supernovae:Individual:SN2023ixf
title_short Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
title_full Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
title_fullStr Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
title_full_unstemmed Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
title_sort Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star
dc.creator.none.fl_str_mv Fang, Qiliang
Moriya, Takashi J.
Ferrari, Lucía
Maeda, Keiichi
Folatelli, Gaston
Ertini, Keila Yael
Kuncarayakti, Hanindyo
Andrews, Jennifer E.
Matsumoto, Tatsuya
author Fang, Qiliang
author_facet Fang, Qiliang
Moriya, Takashi J.
Ferrari, Lucía
Maeda, Keiichi
Folatelli, Gaston
Ertini, Keila Yael
Kuncarayakti, Hanindyo
Andrews, Jennifer E.
Matsumoto, Tatsuya
author_role author
author2 Moriya, Takashi J.
Ferrari, Lucía
Maeda, Keiichi
Folatelli, Gaston
Ertini, Keila Yael
Kuncarayakti, Hanindyo
Andrews, Jennifer E.
Matsumoto, Tatsuya
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Supernovae:general
Supernovae:Individual:SN2023ixf
topic Supernovae:general
Supernovae:Individual:SN2023ixf
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv SN 2023ixf is one of the most well-observed core-collapse supernovae in recent decades, yet there is inconsistencyin the inferred zero-age main-sequence (ZAMS) mass MZAMS of its progenitor. Direct observations of the pre-supernova (SN) red supergiant (RSG) estimate MZAMS spanning widely from 11 to 18 Me. Additional constraints,including the host environment and the pulsation of its progenitor RSG, suggest a massive progenitor withMZAMS > 17 Me. However, the analysis of the SN properties, from light-curve modeling to late-phasespectroscopy, favors a relatively low-mass scenario (MZAMS < 15 Me). In this work, we conduct a systematicanalysis of SN 2023ixf, from the RSG progenitor, plateau phase light curve to late-phase spectroscopy. UsingMESA+STELLA to simulate the RSG progenitor and their explosions, we find that a range of the RSG modelshaving MZAMS that vary from 12 to 17.5 Me can reproduce its multiband light curves if the hydrogen-rich envelopemass and the explosion energy are allowed to vary. Using late-phase spectroscopy as an independent measurement,the oxygen line [O I] indicates an intermediate-massive progenitor (MZAMS ∼ 16.0 Me). By incorporating thevelocity structure derived from the light-curve modeling into an axisymmetric model, we generated [O I] lineprofiles that are consistent with the [O I] line observed in late-phase spectroscopy of SN 2023ixf. Bringing theseanalyses together, we conclude that SN 2023ixf is the aspherical explosion of an intermediate-massive star(MZAMS = 15–16 Me), with the hydrogen envelope being stripped to 4–5 Me prior to its explosion.
Fil: Fang, Qiliang. National Institutes of Natural Sciences; Japón
Fil: Moriya, Takashi J.. National Institutes of Natural Sciences; Japón
Fil: Ferrari, Lucía. 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: Maeda, Keiichi. National Institutes of Natural Sciences; Japón
Fil: Folatelli, Gaston. 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: Ertini, Keila Yael. 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: Kuncarayakti, Hanindyo. University of Turku; Finlandia
Fil: Andrews, Jennifer E.. No especifíca;
Fil: Matsumoto, Tatsuya. Kyoto University; Japón
description SN 2023ixf is one of the most well-observed core-collapse supernovae in recent decades, yet there is inconsistencyin the inferred zero-age main-sequence (ZAMS) mass MZAMS of its progenitor. Direct observations of the pre-supernova (SN) red supergiant (RSG) estimate MZAMS spanning widely from 11 to 18 Me. Additional constraints,including the host environment and the pulsation of its progenitor RSG, suggest a massive progenitor withMZAMS > 17 Me. However, the analysis of the SN properties, from light-curve modeling to late-phasespectroscopy, favors a relatively low-mass scenario (MZAMS < 15 Me). In this work, we conduct a systematicanalysis of SN 2023ixf, from the RSG progenitor, plateau phase light curve to late-phase spectroscopy. UsingMESA+STELLA to simulate the RSG progenitor and their explosions, we find that a range of the RSG modelshaving MZAMS that vary from 12 to 17.5 Me can reproduce its multiband light curves if the hydrogen-rich envelopemass and the explosion energy are allowed to vary. Using late-phase spectroscopy as an independent measurement,the oxygen line [O I] indicates an intermediate-massive progenitor (MZAMS ∼ 16.0 Me). By incorporating thevelocity structure derived from the light-curve modeling into an axisymmetric model, we generated [O I] lineprofiles that are consistent with the [O I] line observed in late-phase spectroscopy of SN 2023ixf. Bringing theseanalyses together, we conclude that SN 2023ixf is the aspherical explosion of an intermediate-massive star(MZAMS = 15–16 Me), with the hydrogen envelope being stripped to 4–5 Me prior to its explosion.
publishDate 2024
dc.date.none.fl_str_mv 2024-12
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/11336/266245
Fang, Qiliang; Moriya, Takashi J.; Ferrari, Lucía; Maeda, Keiichi; Folatelli, Gaston; et al.; Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star; IOP Publishing; Astrophysical Journal; 978; 1; 12-2024; 1-10
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/266245
identifier_str_mv Fang, Qiliang; Moriya, Takashi J.; Ferrari, Lucía; Maeda, Keiichi; Folatelli, Gaston; et al.; Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. II. SN 2023ixf as Explosion of Partially Stripped Intermediate Massive Star; IOP Publishing; Astrophysical Journal; 978; 1; 12-2024; 1-10
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/ad8d5a
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad8d5a
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
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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