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
RID-UNRN (UNRN)
Institución
Universidad Nacional de Río Negro
OAI Identificador
oai:rid.unrn.edu.ar:20.500.12049/2833
Acceder
id RIDUNRN_513ea07f368e278bcd2eca66787bb0af
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network_acronym_str RIDUNRN
repository_id_str 4369
network_name_str RID-UNRN (UNRN)
spelling 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 Negro2025-10-23T11:17:03Zoai: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:43692025-10-23 11:17:03.73RID-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
dc.relation.none.fl_str_mv 817
Astrophysical Journal
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:RID-UNRN (UNRN)
instname:Universidad Nacional de Río Negro
reponame_str RID-UNRN (UNRN)
collection RID-UNRN (UNRN)
instname_str Universidad Nacional de Río Negro
repository.name.fl_str_mv RID-UNRN (UNRN) - Universidad Nacional de Río Negro
repository.mail.fl_str_mv rid@unrn.edu.ar
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score 12.982451

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