The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh
- Autores
- Bersten, Melina C.; Benvenuto, Omar G.; Orellana, Mariana Dominga; Nomoto, Ken’ichi
- Año de publicación
- 2016
- Idioma
- español castellano
- Tipo de recurso
- artículo
- Estado
- versión aceptada
- Descripción
- Fil: Bersten, Melina C. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina.
Fil: Bersten, Melina C. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata.
Fil: Bersten, Melina C. Instituto de Astrofísica de La Plata; Argentina
Fil: Benvenuto, Omar G. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina.
Fil: Benvenuto, Omar G. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Benvenuto, Omar G. Instituto de Astrofísica de La Plata; Argentina
Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina.
Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Nomoto, Ken’ichi. University of Tokyo; Japón
Two recently discovered very luminous supernovae (SNe) present stimulating cases to explore the extents of the available theoretical models. SN 2011kl represents the first detection of a supernova explosion associated with an ultra-long duration gamma-ray burst. ASASSN-15lh was even claimed as the most luminous SN ever discovered, challenging the scenarios so far proposed for stellar explosions. Here we use our radiation hydrodynamics code in order to simulate magnetar-powered SNe. To avoid explicitly assuming neutron star properties, we adopt the magnetar luminosity and spin-down timescale as free parameters of the model. We find that the light curve (LC) of SN 2011kl is consistent with a magnetar power source, as previously proposed, but we note that some amount of 56Ni (> 0.08 Msun ) is necessary to explain the low contrast between the LC peak and tail. For the case of ASASSN-15lh, we find physically plausible magnetar parameters that reproduce the overall shape of the LC provided the progenitor mass is relatively large (an ejecta mass of ~ 6 Msun ). The ejecta hydrodynamics of this event is dominated by the magnetar input, while the effect is more moderate for SN 2011kl. We conclude that a magnetar model may be used for the interpretation of these events and that the hydrodynamical modeling is necessary to derive the properties of powerful magnetars and their progenitors. - Materia
-
Astronomía
Gamma Ray Bursts
Supernovae
SN 2011kl
ASASSN-15lh
Astronomía - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de Río Negro
- OAI Identificador
- oai:rid.unrn.edu.ar:20.500.12049/2833
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The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lhBersten, Melina C.Benvenuto, Omar G.Orellana, Mariana DomingaNomoto, Ken’ichiAstronomíaGamma Ray BurstsSupernovaeSN 2011klASASSN-15lhAstronomíaFil: Bersten, Melina C. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina.Fil: Bersten, Melina C. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata.Fil: Bersten, Melina C. Instituto de Astrofísica de La Plata; ArgentinaFil: Benvenuto, Omar G. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina.Fil: Benvenuto, Omar G. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Benvenuto, Omar G. Instituto de Astrofísica de La Plata; ArgentinaFil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina.Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Nomoto, Ken’ichi. University of Tokyo; JapónTwo recently discovered very luminous supernovae (SNe) present stimulating cases to explore the extents of the available theoretical models. SN 2011kl represents the first detection of a supernova explosion associated with an ultra-long duration gamma-ray burst. ASASSN-15lh was even claimed as the most luminous SN ever discovered, challenging the scenarios so far proposed for stellar explosions. Here we use our radiation hydrodynamics code in order to simulate magnetar-powered SNe. To avoid explicitly assuming neutron star properties, we adopt the magnetar luminosity and spin-down timescale as free parameters of the model. We find that the light curve (LC) of SN 2011kl is consistent with a magnetar power source, as previously proposed, but we note that some amount of 56Ni (> 0.08 Msun ) is necessary to explain the low contrast between the LC peak and tail. For the case of ASASSN-15lh, we find physically plausible magnetar parameters that reproduce the overall shape of the LC provided the progenitor mass is relatively large (an ejecta mass of ~ 6 Msun ). The ejecta hydrodynamics of this event is dominated by the magnetar input, while the effect is more moderate for SN 2011kl. We conclude that a magnetar model may be used for the interpretation of these events and that the hydrodynamical modeling is necessary to derive the properties of powerful magnetars and their progenitors.IOP Publishing2016-01-19info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfBersten, Melina C., Benvenuto, Omar G., Orellana, Mariana D. & Nomoto, Ken’ichi. (2016). The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh. IOP Publishing; Astrophysical Journal; 817; p. 1-50004-637X1538-4357http://iopscience.iop.org/article/10.3847/2041-8205/817/1/L8/metahttp://hdl.handle.net/11336/35490https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2833http://dx.doi.org/10.3847/2041-8205/817/1/L8spa817Astrophysical Journalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-09-29T14:28:45Zoai:rid.unrn.edu.ar:20.500.12049/2833instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-09-29 14:28:46.127RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse |
dc.title.none.fl_str_mv |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
title |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
spellingShingle |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh Bersten, Melina C. Astronomía Gamma Ray Bursts Supernovae SN 2011kl ASASSN-15lh Astronomía |
title_short |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
title_full |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
title_fullStr |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
title_full_unstemmed |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
title_sort |
The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh |
dc.creator.none.fl_str_mv |
Bersten, Melina C. Benvenuto, Omar G. Orellana, Mariana Dominga Nomoto, Ken’ichi |
author |
Bersten, Melina C. |
author_facet |
Bersten, Melina C. Benvenuto, Omar G. Orellana, Mariana Dominga Nomoto, Ken’ichi |
author_role |
author |
author2 |
Benvenuto, Omar G. Orellana, Mariana Dominga Nomoto, Ken’ichi |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Astronomía Gamma Ray Bursts Supernovae SN 2011kl ASASSN-15lh Astronomía |
topic |
Astronomía Gamma Ray Bursts Supernovae SN 2011kl ASASSN-15lh Astronomía |
dc.description.none.fl_txt_mv |
Fil: Bersten, Melina C. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Fil: Bersten, Melina C. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Fil: Bersten, Melina C. Instituto de Astrofísica de La Plata; Argentina Fil: Benvenuto, Omar G. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Fil: Benvenuto, Omar G. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Benvenuto, Omar G. Instituto de Astrofísica de La Plata; Argentina Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina. Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Nomoto, Ken’ichi. University of Tokyo; Japón Two recently discovered very luminous supernovae (SNe) present stimulating cases to explore the extents of the available theoretical models. SN 2011kl represents the first detection of a supernova explosion associated with an ultra-long duration gamma-ray burst. ASASSN-15lh was even claimed as the most luminous SN ever discovered, challenging the scenarios so far proposed for stellar explosions. Here we use our radiation hydrodynamics code in order to simulate magnetar-powered SNe. To avoid explicitly assuming neutron star properties, we adopt the magnetar luminosity and spin-down timescale as free parameters of the model. We find that the light curve (LC) of SN 2011kl is consistent with a magnetar power source, as previously proposed, but we note that some amount of 56Ni (> 0.08 Msun ) is necessary to explain the low contrast between the LC peak and tail. For the case of ASASSN-15lh, we find physically plausible magnetar parameters that reproduce the overall shape of the LC provided the progenitor mass is relatively large (an ejecta mass of ~ 6 Msun ). The ejecta hydrodynamics of this event is dominated by the magnetar input, while the effect is more moderate for SN 2011kl. We conclude that a magnetar model may be used for the interpretation of these events and that the hydrodynamical modeling is necessary to derive the properties of powerful magnetars and their progenitors. |
description |
Fil: Bersten, Melina C. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-01-19 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
acceptedVersion |
dc.identifier.none.fl_str_mv |
Bersten, Melina C., Benvenuto, Omar G., Orellana, Mariana D. & Nomoto, Ken’ichi. (2016). The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh. IOP Publishing; Astrophysical Journal; 817; p. 1-5 0004-637X 1538-4357 http://iopscience.iop.org/article/10.3847/2041-8205/817/1/L8/meta http://hdl.handle.net/11336/35490 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2833 http://dx.doi.org/10.3847/2041-8205/817/1/L8 |
identifier_str_mv |
Bersten, Melina C., Benvenuto, Omar G., Orellana, Mariana D. & Nomoto, Ken’ichi. (2016). The Unusual Super-luminous Supernovae SN 2011kl and ASASSN-15lh. IOP Publishing; Astrophysical Journal; 817; p. 1-5 0004-637X 1538-4357 |
url |
http://iopscience.iop.org/article/10.3847/2041-8205/817/1/L8/meta http://hdl.handle.net/11336/35490 https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2833 http://dx.doi.org/10.3847/2041-8205/817/1/L8 |
dc.language.none.fl_str_mv |
spa |
language |
spa |
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817 Astrophysical Journal |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/4.0/ |
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IOP Publishing |
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IOP Publishing |
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