The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi

Autores
Maeda, Keiichi; Chandra, Poonam; Matsuoka, Tomoki; Ryder, Stuart; Moriya, Takashi J.; Kuncarayakti, Hanindyo; Lee, Shiu Hang; Kundu, Esha; Patnaude, Daniel; Saito, Tomoki; Folatelli, Gaston
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the results of Atacama Large Millimeter/submillimeter Array (ALMA) band 3 observations of the nearby type Ic supernova (SN) 2020oi. Under the standard assumptions on the SN-circumstellar medium (CSM) interaction and the synchrotron emission, the data indicate that the CSM structure deviates from a smooth distribution expected from the steady-state mass loss in the very vicinity of the SN (≲1015 cm), which is then connected to the outer smooth distribution (⪆1016 cm). This structure is further confirmed through the light-curve modeling of the whole radio data set as combined with the previously reported data at lower frequency. Because this is an explosion of a bare carbon-oxygen (C+O) star with a fast wind, we can trace the mass-loss history of the progenitor of SN 2020oi in the final year. The inferred nonsmooth CSM distribution corresponds to fluctuations on the subyear timescale in the mass-loss history toward the SN explosion. Our finding suggests that the pre-SN activity is likely driven by the accelerated change in the nuclear burning stage in the last moments just before the massive star´s demise. The structure of the CSM derived in this study is beyond the applicability of the other methods at optical wavelengths, highlighting the importance and uniqueness of quick follow-up observations of SNe by ALMA and other radio facilities.
Fil: Maeda, Keiichi. Kyoto University; Japón
Fil: Chandra, Poonam. National Centre For Radio Astrophysics India; India
Fil: Matsuoka, Tomoki. Kyoto University; Japón
Fil: Ryder, Stuart. Macquarie University; Australia
Fil: Moriya, Takashi J.. Monash University; Australia
Fil: Kuncarayakti, Hanindyo. University of Turku; Finlandia
Fil: Lee, Shiu Hang. Kyoto University; Japón
Fil: Kundu, Esha. Curtin University; Australia
Fil: Patnaude, Daniel. Smithsonian Astrophysical Observatory; Estados Unidos
Fil: Saito, Tomoki. University Of Hyogo; 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
Materia
SUPERNOVAE
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:11336/169341
Acceder
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network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oiMaeda, KeiichiChandra, PoonamMatsuoka, TomokiRyder, StuartMoriya, Takashi J.Kuncarayakti, HanindyoLee, Shiu HangKundu, EshaPatnaude, DanielSaito, TomokiFolatelli, GastonSUPERNOVAEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the results of Atacama Large Millimeter/submillimeter Array (ALMA) band 3 observations of the nearby type Ic supernova (SN) 2020oi. Under the standard assumptions on the SN-circumstellar medium (CSM) interaction and the synchrotron emission, the data indicate that the CSM structure deviates from a smooth distribution expected from the steady-state mass loss in the very vicinity of the SN (≲1015 cm), which is then connected to the outer smooth distribution (⪆1016 cm). This structure is further confirmed through the light-curve modeling of the whole radio data set as combined with the previously reported data at lower frequency. Because this is an explosion of a bare carbon-oxygen (C+O) star with a fast wind, we can trace the mass-loss history of the progenitor of SN 2020oi in the final year. The inferred nonsmooth CSM distribution corresponds to fluctuations on the subyear timescale in the mass-loss history toward the SN explosion. Our finding suggests that the pre-SN activity is likely driven by the accelerated change in the nuclear burning stage in the last moments just before the massive star´s demise. The structure of the CSM derived in this study is beyond the applicability of the other methods at optical wavelengths, highlighting the importance and uniqueness of quick follow-up observations of SNe by ALMA and other radio facilities.Fil: Maeda, Keiichi. Kyoto University; JapónFil: Chandra, Poonam. National Centre For Radio Astrophysics India; IndiaFil: Matsuoka, Tomoki. Kyoto University; JapónFil: Ryder, Stuart. Macquarie University; AustraliaFil: Moriya, Takashi J.. Monash University; AustraliaFil: Kuncarayakti, Hanindyo. University of Turku; FinlandiaFil: Lee, Shiu Hang. Kyoto University; JapónFil: Kundu, Esha. Curtin University; AustraliaFil: Patnaude, Daniel. Smithsonian Astrophysical Observatory; Estados UnidosFil: Saito, Tomoki. University Of Hyogo; 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; ArgentinaIOP Publishing2021-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/169341Maeda, Keiichi; Chandra, Poonam; Matsuoka, Tomoki; Ryder, Stuart; Moriya, Takashi J.; et al.; The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi; IOP Publishing; Astrophysical Journal; 918; 1; 9-2021; 1-200004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ac0dbcinfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac0dbcinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:35:10Zoai:ri.conicet.gov.ar:11336/169341instacron: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 10:35:10.306CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
title The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
spellingShingle The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
Maeda, Keiichi
SUPERNOVAE
title_short The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
title_full The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
title_fullStr The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
title_full_unstemmed The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
title_sort The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi
dc.creator.none.fl_str_mv Maeda, Keiichi
Chandra, Poonam
Matsuoka, Tomoki
Ryder, Stuart
Moriya, Takashi J.
Kuncarayakti, Hanindyo
Lee, Shiu Hang
Kundu, Esha
Patnaude, Daniel
Saito, Tomoki
Folatelli, Gaston
author Maeda, Keiichi
author_facet Maeda, Keiichi
Chandra, Poonam
Matsuoka, Tomoki
Ryder, Stuart
Moriya, Takashi J.
Kuncarayakti, Hanindyo
Lee, Shiu Hang
Kundu, Esha
Patnaude, Daniel
Saito, Tomoki
Folatelli, Gaston
author_role author
author2 Chandra, Poonam
Matsuoka, Tomoki
Ryder, Stuart
Moriya, Takashi J.
Kuncarayakti, Hanindyo
Lee, Shiu Hang
Kundu, Esha
Patnaude, Daniel
Saito, Tomoki
Folatelli, Gaston
author2_role author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv SUPERNOVAE
topic SUPERNOVAE
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present the results of Atacama Large Millimeter/submillimeter Array (ALMA) band 3 observations of the nearby type Ic supernova (SN) 2020oi. Under the standard assumptions on the SN-circumstellar medium (CSM) interaction and the synchrotron emission, the data indicate that the CSM structure deviates from a smooth distribution expected from the steady-state mass loss in the very vicinity of the SN (≲1015 cm), which is then connected to the outer smooth distribution (⪆1016 cm). This structure is further confirmed through the light-curve modeling of the whole radio data set as combined with the previously reported data at lower frequency. Because this is an explosion of a bare carbon-oxygen (C+O) star with a fast wind, we can trace the mass-loss history of the progenitor of SN 2020oi in the final year. The inferred nonsmooth CSM distribution corresponds to fluctuations on the subyear timescale in the mass-loss history toward the SN explosion. Our finding suggests that the pre-SN activity is likely driven by the accelerated change in the nuclear burning stage in the last moments just before the massive star´s demise. The structure of the CSM derived in this study is beyond the applicability of the other methods at optical wavelengths, highlighting the importance and uniqueness of quick follow-up observations of SNe by ALMA and other radio facilities.
Fil: Maeda, Keiichi. Kyoto University; Japón
Fil: Chandra, Poonam. National Centre For Radio Astrophysics India; India
Fil: Matsuoka, Tomoki. Kyoto University; Japón
Fil: Ryder, Stuart. Macquarie University; Australia
Fil: Moriya, Takashi J.. Monash University; Australia
Fil: Kuncarayakti, Hanindyo. University of Turku; Finlandia
Fil: Lee, Shiu Hang. Kyoto University; Japón
Fil: Kundu, Esha. Curtin University; Australia
Fil: Patnaude, Daniel. Smithsonian Astrophysical Observatory; Estados Unidos
Fil: Saito, Tomoki. University Of Hyogo; 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
description We present the results of Atacama Large Millimeter/submillimeter Array (ALMA) band 3 observations of the nearby type Ic supernova (SN) 2020oi. Under the standard assumptions on the SN-circumstellar medium (CSM) interaction and the synchrotron emission, the data indicate that the CSM structure deviates from a smooth distribution expected from the steady-state mass loss in the very vicinity of the SN (≲1015 cm), which is then connected to the outer smooth distribution (⪆1016 cm). This structure is further confirmed through the light-curve modeling of the whole radio data set as combined with the previously reported data at lower frequency. Because this is an explosion of a bare carbon-oxygen (C+O) star with a fast wind, we can trace the mass-loss history of the progenitor of SN 2020oi in the final year. The inferred nonsmooth CSM distribution corresponds to fluctuations on the subyear timescale in the mass-loss history toward the SN explosion. Our finding suggests that the pre-SN activity is likely driven by the accelerated change in the nuclear burning stage in the last moments just before the massive star´s demise. The structure of the CSM derived in this study is beyond the applicability of the other methods at optical wavelengths, highlighting the importance and uniqueness of quick follow-up observations of SNe by ALMA and other radio facilities.
publishDate 2021
dc.date.none.fl_str_mv 2021-09
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/11336/169341
Maeda, Keiichi; Chandra, Poonam; Matsuoka, Tomoki; Ryder, Stuart; Moriya, Takashi J.; et al.; The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi; IOP Publishing; Astrophysical Journal; 918; 1; 9-2021; 1-20
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/169341
identifier_str_mv Maeda, Keiichi; Chandra, Poonam; Matsuoka, Tomoki; Ryder, Stuart; Moriya, Takashi J.; et al.; The Final Months of Massive Star Evolution from the Circumstellar Environment around SN Ic 2020oi; IOP Publishing; Astrophysical Journal; 918; 1; 9-2021; 1-20
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/doi/10.3847/1538-4357/ac0dbc
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ac0dbc
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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