Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
- Autores
- Hiramatsu, Daichi; Howell, D. Andrew; Moriya, Takashi J.; Goldberg, Jared A.; Hosseinzadeh, Griffin; Arcavi, Iair; Anderson, Joseph; Gutiérrez, Claudia P.; Burke, Jamison; McCully, Curtis; Valenti, Stefano; Galbany, Lluís; Fang, Qiliang; Maeda, Keiichi; Folatelli, Gaston; Hsiao, Eric Y.; Morrell, Nidia Irene; Phillips, Mark M.; Stritzinger, Maximilian D.; Suntzeff, Nicholas B.; Gromadzki, Mariusz; Maguire, Kate; Müller Bravo, Tomás E.; Young, David R.
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor´s hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plateaus (∼100 days) and the most massive H-rich envelopes. However, it is an ongoing mystery why SNe II with short plateaus (tens of days) are rarely seen. Here, we present optical/near-infrared photometric and spectroscopic observations of luminous Type II short-plateau SNe 2006Y, 2006ai, and 2016egz. Their plateaus of about 50-70 days and luminous optical peaks (≲-18.4 mag) indicate significant pre-explosion mass loss resulting in partially stripped H-rich envelopes and early circumstellar material (CSM) interaction. We compute a large grid of MESA+STELLA single-star progenitor and light-curve models with various progenitor zero-age main-sequence (ZAMS) masses, mass-loss efficiencies, explosion energies, 56Ni masses, and CSM densities. Our model grid shows a continuous population of SNe IIP-IIL-IIb-like light-curve morphology in descending order of H-rich envelope mass. With large 56Ni masses (⪆0.05 M o˙), short-plateau SNe II lie in a confined parameter space as a transitional class between SNe IIL and IIb. For SNe 2006Y, 2006ai, and 2016egz, our findings suggest high-mass red supergiant (RSG) progenitors (M ZAMS ≃ 18-22 M o˙) with small H-rich envelope masses () that have experienced enhanced mass loss () for the last few decades before the explosion. If high-mass RSGs result in rare short-plateau SNe II, then these events might ease some of the apparent underrepresentation of higher-luminosity RSGs in observed SN II progenitor samples.
Fil: Hiramatsu, Daichi. University of California; Estados Unidos
Fil: Howell, D. Andrew. University of California; Estados Unidos
Fil: Moriya, Takashi J.. Monash University; Australia
Fil: Goldberg, Jared A.. University of California; Estados Unidos
Fil: Hosseinzadeh, Griffin. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Arcavi, Iair. Tel Aviv University; Israel
Fil: Anderson, Joseph. European Southern Observatory Santiago; Chile
Fil: Gutiérrez, Claudia P.. University of Southampton; Reino Unido
Fil: Burke, Jamison. University of California; Estados Unidos
Fil: McCully, Curtis. University of California; Estados Unidos
Fil: Valenti, Stefano. University of California at Davis; Estados Unidos
Fil: Galbany, Lluís. Universidad de Granada; España
Fil: Fang, Qiliang. Kyoto University; Japón
Fil: Maeda, Keiichi. The University Of Tokyo; 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: Hsiao, Eric Y.. Florida State University; Estados Unidos
Fil: Morrell, Nidia Irene. Las Campanas Observatory; Chile
Fil: Phillips, Mark M.. Las Campanas Observatory; Chile
Fil: Stritzinger, Maximilian D.. University Aarhus; Dinamarca
Fil: Suntzeff, Nicholas B.. Texas A&M University; Estados Unidos
Fil: Gromadzki, Mariusz. University of Warsaw; Polonia
Fil: Maguire, Kate. Trinity College Dublin; Irlanda
Fil: Müller Bravo, Tomás E.. University of Southampton; Reino Unido
Fil: Young, David R.. The Queens University of Belfast; Irlanda - Materia
- SUPERNOVAE
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/167603
Ver los metadatos del registro completo
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Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red SupergiantsHiramatsu, DaichiHowell, D. AndrewMoriya, Takashi J.Goldberg, Jared A.Hosseinzadeh, GriffinArcavi, IairAnderson, JosephGutiérrez, Claudia P.Burke, JamisonMcCully, CurtisValenti, StefanoGalbany, LluísFang, QiliangMaeda, KeiichiFolatelli, GastonHsiao, Eric Y.Morrell, Nidia IrenePhillips, Mark M.Stritzinger, Maximilian D.Suntzeff, Nicholas B.Gromadzki, MariuszMaguire, KateMüller Bravo, Tomás E.Young, David R.SUPERNOVAEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor´s hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plateaus (∼100 days) and the most massive H-rich envelopes. However, it is an ongoing mystery why SNe II with short plateaus (tens of days) are rarely seen. Here, we present optical/near-infrared photometric and spectroscopic observations of luminous Type II short-plateau SNe 2006Y, 2006ai, and 2016egz. Their plateaus of about 50-70 days and luminous optical peaks (≲-18.4 mag) indicate significant pre-explosion mass loss resulting in partially stripped H-rich envelopes and early circumstellar material (CSM) interaction. We compute a large grid of MESA+STELLA single-star progenitor and light-curve models with various progenitor zero-age main-sequence (ZAMS) masses, mass-loss efficiencies, explosion energies, 56Ni masses, and CSM densities. Our model grid shows a continuous population of SNe IIP-IIL-IIb-like light-curve morphology in descending order of H-rich envelope mass. With large 56Ni masses (⪆0.05 M o˙), short-plateau SNe II lie in a confined parameter space as a transitional class between SNe IIL and IIb. For SNe 2006Y, 2006ai, and 2016egz, our findings suggest high-mass red supergiant (RSG) progenitors (M ZAMS ≃ 18-22 M o˙) with small H-rich envelope masses () that have experienced enhanced mass loss () for the last few decades before the explosion. If high-mass RSGs result in rare short-plateau SNe II, then these events might ease some of the apparent underrepresentation of higher-luminosity RSGs in observed SN II progenitor samples.Fil: Hiramatsu, Daichi. University of California; Estados UnidosFil: Howell, D. Andrew. University of California; Estados UnidosFil: Moriya, Takashi J.. Monash University; AustraliaFil: Goldberg, Jared A.. University of California; Estados UnidosFil: Hosseinzadeh, Griffin. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Arcavi, Iair. Tel Aviv University; IsraelFil: Anderson, Joseph. European Southern Observatory Santiago; ChileFil: Gutiérrez, Claudia P.. University of Southampton; Reino UnidoFil: Burke, Jamison. University of California; Estados UnidosFil: McCully, Curtis. University of California; Estados UnidosFil: Valenti, Stefano. University of California at Davis; Estados UnidosFil: Galbany, Lluís. Universidad de Granada; EspañaFil: Fang, Qiliang. Kyoto University; JapónFil: Maeda, Keiichi. The University Of Tokyo; 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: Hsiao, Eric Y.. Florida State University; Estados UnidosFil: Morrell, Nidia Irene. Las Campanas Observatory; ChileFil: Phillips, Mark M.. Las Campanas Observatory; ChileFil: Stritzinger, Maximilian D.. University Aarhus; DinamarcaFil: Suntzeff, Nicholas B.. Texas A&M University; Estados UnidosFil: Gromadzki, Mariusz. University of Warsaw; PoloniaFil: Maguire, Kate. Trinity College Dublin; IrlandaFil: Müller Bravo, Tomás E.. University of Southampton; Reino UnidoFil: Young, David R.. The Queens University of Belfast; IrlandaIOP Publishing2021-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/167603Hiramatsu, Daichi; Howell, D. Andrew; Moriya, Takashi J.; Goldberg, Jared A.; Hosseinzadeh, Griffin; et al.; Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants; IOP Publishing; Astrophysical Journal; 913; 1; 5-2021; 1-270004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/abf6d6info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/abf6d6info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-01-14T11:43:27Zoai:ri.conicet.gov.ar:11336/167603instacron: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:34982026-01-14 11:43:27.685CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| title |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| spellingShingle |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants Hiramatsu, Daichi SUPERNOVAE |
| title_short |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| title_full |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| title_fullStr |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| title_full_unstemmed |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| title_sort |
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants |
| dc.creator.none.fl_str_mv |
Hiramatsu, Daichi Howell, D. Andrew Moriya, Takashi J. Goldberg, Jared A. Hosseinzadeh, Griffin Arcavi, Iair Anderson, Joseph Gutiérrez, Claudia P. Burke, Jamison McCully, Curtis Valenti, Stefano Galbany, Lluís Fang, Qiliang Maeda, Keiichi Folatelli, Gaston Hsiao, Eric Y. Morrell, Nidia Irene Phillips, Mark M. Stritzinger, Maximilian D. Suntzeff, Nicholas B. Gromadzki, Mariusz Maguire, Kate Müller Bravo, Tomás E. Young, David R. |
| author |
Hiramatsu, Daichi |
| author_facet |
Hiramatsu, Daichi Howell, D. Andrew Moriya, Takashi J. Goldberg, Jared A. Hosseinzadeh, Griffin Arcavi, Iair Anderson, Joseph Gutiérrez, Claudia P. Burke, Jamison McCully, Curtis Valenti, Stefano Galbany, Lluís Fang, Qiliang Maeda, Keiichi Folatelli, Gaston Hsiao, Eric Y. Morrell, Nidia Irene Phillips, Mark M. Stritzinger, Maximilian D. Suntzeff, Nicholas B. Gromadzki, Mariusz Maguire, Kate Müller Bravo, Tomás E. Young, David R. |
| author_role |
author |
| author2 |
Howell, D. Andrew Moriya, Takashi J. Goldberg, Jared A. Hosseinzadeh, Griffin Arcavi, Iair Anderson, Joseph Gutiérrez, Claudia P. Burke, Jamison McCully, Curtis Valenti, Stefano Galbany, Lluís Fang, Qiliang Maeda, Keiichi Folatelli, Gaston Hsiao, Eric Y. Morrell, Nidia Irene Phillips, Mark M. Stritzinger, Maximilian D. Suntzeff, Nicholas B. Gromadzki, Mariusz Maguire, Kate Müller Bravo, Tomás E. Young, David R. |
| author2_role |
author 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 |
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 |
The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor´s hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plateaus (∼100 days) and the most massive H-rich envelopes. However, it is an ongoing mystery why SNe II with short plateaus (tens of days) are rarely seen. Here, we present optical/near-infrared photometric and spectroscopic observations of luminous Type II short-plateau SNe 2006Y, 2006ai, and 2016egz. Their plateaus of about 50-70 days and luminous optical peaks (≲-18.4 mag) indicate significant pre-explosion mass loss resulting in partially stripped H-rich envelopes and early circumstellar material (CSM) interaction. We compute a large grid of MESA+STELLA single-star progenitor and light-curve models with various progenitor zero-age main-sequence (ZAMS) masses, mass-loss efficiencies, explosion energies, 56Ni masses, and CSM densities. Our model grid shows a continuous population of SNe IIP-IIL-IIb-like light-curve morphology in descending order of H-rich envelope mass. With large 56Ni masses (⪆0.05 M o˙), short-plateau SNe II lie in a confined parameter space as a transitional class between SNe IIL and IIb. For SNe 2006Y, 2006ai, and 2016egz, our findings suggest high-mass red supergiant (RSG) progenitors (M ZAMS ≃ 18-22 M o˙) with small H-rich envelope masses () that have experienced enhanced mass loss () for the last few decades before the explosion. If high-mass RSGs result in rare short-plateau SNe II, then these events might ease some of the apparent underrepresentation of higher-luminosity RSGs in observed SN II progenitor samples. Fil: Hiramatsu, Daichi. University of California; Estados Unidos Fil: Howell, D. Andrew. University of California; Estados Unidos Fil: Moriya, Takashi J.. Monash University; Australia Fil: Goldberg, Jared A.. University of California; Estados Unidos Fil: Hosseinzadeh, Griffin. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Arcavi, Iair. Tel Aviv University; Israel Fil: Anderson, Joseph. European Southern Observatory Santiago; Chile Fil: Gutiérrez, Claudia P.. University of Southampton; Reino Unido Fil: Burke, Jamison. University of California; Estados Unidos Fil: McCully, Curtis. University of California; Estados Unidos Fil: Valenti, Stefano. University of California at Davis; Estados Unidos Fil: Galbany, Lluís. Universidad de Granada; España Fil: Fang, Qiliang. Kyoto University; Japón Fil: Maeda, Keiichi. The University Of Tokyo; 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: Hsiao, Eric Y.. Florida State University; Estados Unidos Fil: Morrell, Nidia Irene. Las Campanas Observatory; Chile Fil: Phillips, Mark M.. Las Campanas Observatory; Chile Fil: Stritzinger, Maximilian D.. University Aarhus; Dinamarca Fil: Suntzeff, Nicholas B.. Texas A&M University; Estados Unidos Fil: Gromadzki, Mariusz. University of Warsaw; Polonia Fil: Maguire, Kate. Trinity College Dublin; Irlanda Fil: Müller Bravo, Tomás E.. University of Southampton; Reino Unido Fil: Young, David R.. The Queens University of Belfast; Irlanda |
| description |
The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor´s hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plateaus (∼100 days) and the most massive H-rich envelopes. However, it is an ongoing mystery why SNe II with short plateaus (tens of days) are rarely seen. Here, we present optical/near-infrared photometric and spectroscopic observations of luminous Type II short-plateau SNe 2006Y, 2006ai, and 2016egz. Their plateaus of about 50-70 days and luminous optical peaks (≲-18.4 mag) indicate significant pre-explosion mass loss resulting in partially stripped H-rich envelopes and early circumstellar material (CSM) interaction. We compute a large grid of MESA+STELLA single-star progenitor and light-curve models with various progenitor zero-age main-sequence (ZAMS) masses, mass-loss efficiencies, explosion energies, 56Ni masses, and CSM densities. Our model grid shows a continuous population of SNe IIP-IIL-IIb-like light-curve morphology in descending order of H-rich envelope mass. With large 56Ni masses (⪆0.05 M o˙), short-plateau SNe II lie in a confined parameter space as a transitional class between SNe IIL and IIb. For SNe 2006Y, 2006ai, and 2016egz, our findings suggest high-mass red supergiant (RSG) progenitors (M ZAMS ≃ 18-22 M o˙) with small H-rich envelope masses () that have experienced enhanced mass loss () for the last few decades before the explosion. If high-mass RSGs result in rare short-plateau SNe II, then these events might ease some of the apparent underrepresentation of higher-luminosity RSGs in observed SN II progenitor samples. |
| publishDate |
2021 |
| dc.date.none.fl_str_mv |
2021-05 |
| 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/11336/167603 Hiramatsu, Daichi; Howell, D. Andrew; Moriya, Takashi J.; Goldberg, Jared A.; Hosseinzadeh, Griffin; et al.; Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants; IOP Publishing; Astrophysical Journal; 913; 1; 5-2021; 1-27 0004-637X CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/167603 |
| identifier_str_mv |
Hiramatsu, Daichi; Howell, D. Andrew; Moriya, Takashi J.; Goldberg, Jared A.; Hosseinzadeh, Griffin; et al.; Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants; IOP Publishing; Astrophysical Journal; 913; 1; 5-2021; 1-27 0004-637X CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/abf6d6 info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/abf6d6 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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application/pdf application/pdf |
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IOP Publishing |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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