The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D
- Autores
- Bufano, Filomena; Pian, Elena; Sollerman, Jesper; Benetti, Stefano; Pignata, Giuliano; Valenti, Stefano; Covino, Stefano; D´Avanzo, Paolo; Malesani, Daniele; Cappellaro, Enrico; Della Valle, Massimo; Fynbo, Johan; Hjorth, Jens; Mazzali, Paolo, A.; Reichart, Daniel E.; Starling, Rhaana L. C.; Turatto, Massimo; Vergani, Susanna D.; Wiersema, Klass; Amati, Lorenzo; Bersier, David; Campana, Sergio; Cano, Zach; Castro Tirado, Alberto J.; Chincarini, Guido; D´Elia, Valerio; de Ugarte Postigo, Antonio; Deng, Jinsong; Ferrero, Patricia; Mirabel Miquele, Igor Felix
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed Type Ic supernova, SN 2010bh, associated with the soft, long-duration gamma-ray burst (X-ray flash) GRB 100316D. Intensive follow-up observations of SN 2010bh were performed at the ESO Very Large Telescope (VLT) using the X-shooter and FORS2 instruments. Thanks to the detailed temporal coverage and the extended wavelength range (3000-24800 Å), we obtained an unprecedentedly rich spectral sequence among the hypernovae, making SN 2010bh one of the best studied representatives of this SN class. We find that SN 2010bh has a more rapid rise to maximum brightness (8.0 ± 1.0 rest-frame days) and a fainter absolute peak luminosity (L bol ≈ 3 × 1042 erg s–1) than previously observed SN events associated with GRBs. Our estimate of the ejected 56Ni mass is 0.12 ± 0.02 M ☉. From the broad spectral features, we measure expansion velocities up to 47,000 km s–1, higher than those of SNe 1998bw (GRB 980425) and 2006aj (GRB 060218). Helium absorption lines He I λ5876 and He I 1.083 μm, blueshifted by ~20,000-30,000 km s–1 and ~28,000-38,000 km s–1, respectively, may be present in the optical spectra. However, the lack of coverage of the He I 2.058 μm line prevents us from confirming such identifications. The nebular spectrum, taken at ~186 days after the explosion, shows a broad but faint [O I] emission at 6340 Å. The light curve shape and photospheric expansion velocities of SN 2010bh suggest that we witnessed a highly energetic explosion with a small ejected mass (E k ≈ 1052 erg and M ej ≈ 3 M ☉). The observed properties of SN 2010bh further extend the heterogeneity of the class of GRB SNe.
Fil: Bufano, Filomena. Osservatorio Astronomico di Catania; Italia
Fil: Pian, Elena. Osservatorio Astronomico di Trieste; Italia
Fil: Sollerman, Jesper. The Oskar Klein Centre; Suecia
Fil: Benetti, Stefano. Osservatorio Astronomico di Padova; Italia
Fil: Pignata, Giuliano. Universidad Andres Bello; Chile
Fil: Valenti, Stefano. Osservatorio Astronomico di Padova; Italia
Fil: Covino, Stefano. Osservatorio Astronomico di Brera; Italia
Fil: D´Avanzo, Paolo. Osservatorio Astronomico di Brera; Italia
Fil: Malesani, Daniele. University of Copenhagen; Dinamarca
Fil: Cappellaro, Enrico. Osservatorio Astronomico di Padova; Italia
Fil: Della Valle, Massimo. Osservatorio Astronomico di Capodimonte; Italia
Fil: Fynbo, Johan. Universidad de Copenhagen; Dinamarca
Fil: Hjorth, Jens. Universidad de Copenhagen; Dinamarca
Fil: Mazzali, Paolo, A.. Osservatorio Astronomico di Padova; Italia
Fil: Reichart, Daniel E.. University of North Carolina; Estados Unidos
Fil: Starling, Rhaana L. C.. University of Leicester; Reino Unido
Fil: Turatto, Massimo. Osservatorio Astronomico di Trieste; Italia
Fil: Vergani, Susanna D.. Osservatorio Astronomico di Brera; Italia
Fil: Wiersema, Klass. University of Leicester; Reino Unido
Fil: Amati, Lorenzo. Istituto di Astrofisica Spaziale e Fisica cosmica; Italia
Fil: Bersier, David. Liverpool John Moores University; Reino Unido
Fil: Campana, Sergio. Osservatorio Astronomico di Brera; Italia
Fil: Cano, Zach. Liverpool John Moores University; Reino Unido
Fil: Castro Tirado, Alberto J.. Instituto de Astrofisica de Andalucia; España
Fil: Chincarini, Guido. Univerisit Milano Bicocca; Italia
Fil: D´Elia, Valerio. Osservatorio Astronomico di Roma; Italia
Fil: de Ugarte Postigo, Antonio. Universidad de Copenhagen; Dinamarca
Fil: Deng, Jinsong. National Astronomical Observatories; China
Fil: Ferrero, Patricia. Instituto de Astrofsica de Canarias; España
Fil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina - Materia
-
supernovae: general
supernovae: individual:
SN 2010bh GRB 100316D - 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:11336/21217
Ver los metadatos del registro completo
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The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316DBufano, FilomenaPian, ElenaSollerman, JesperBenetti, StefanoPignata, GiulianoValenti, StefanoCovino, StefanoD´Avanzo, PaoloMalesani, DanieleCappellaro, EnricoDella Valle, MassimoFynbo, JohanHjorth, JensMazzali, Paolo, A.Reichart, Daniel E.Starling, Rhaana L. C.Turatto, MassimoVergani, Susanna D.Wiersema, KlassAmati, LorenzoBersier, DavidCampana, SergioCano, ZachCastro Tirado, Alberto J.Chincarini, GuidoD´Elia, Valeriode Ugarte Postigo, AntonioDeng, JinsongFerrero, PatriciaMirabel Miquele, Igor Felixsupernovae: generalsupernovae: individual:SN 2010bh GRB 100316Dhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed Type Ic supernova, SN 2010bh, associated with the soft, long-duration gamma-ray burst (X-ray flash) GRB 100316D. Intensive follow-up observations of SN 2010bh were performed at the ESO Very Large Telescope (VLT) using the X-shooter and FORS2 instruments. Thanks to the detailed temporal coverage and the extended wavelength range (3000-24800 Å), we obtained an unprecedentedly rich spectral sequence among the hypernovae, making SN 2010bh one of the best studied representatives of this SN class. We find that SN 2010bh has a more rapid rise to maximum brightness (8.0 ± 1.0 rest-frame days) and a fainter absolute peak luminosity (L bol ≈ 3 × 1042 erg s–1) than previously observed SN events associated with GRBs. Our estimate of the ejected 56Ni mass is 0.12 ± 0.02 M ☉. From the broad spectral features, we measure expansion velocities up to 47,000 km s–1, higher than those of SNe 1998bw (GRB 980425) and 2006aj (GRB 060218). Helium absorption lines He I λ5876 and He I 1.083 μm, blueshifted by ~20,000-30,000 km s–1 and ~28,000-38,000 km s–1, respectively, may be present in the optical spectra. However, the lack of coverage of the He I 2.058 μm line prevents us from confirming such identifications. The nebular spectrum, taken at ~186 days after the explosion, shows a broad but faint [O I] emission at 6340 Å. The light curve shape and photospheric expansion velocities of SN 2010bh suggest that we witnessed a highly energetic explosion with a small ejected mass (E k ≈ 1052 erg and M ej ≈ 3 M ☉). The observed properties of SN 2010bh further extend the heterogeneity of the class of GRB SNe.Fil: Bufano, Filomena. Osservatorio Astronomico di Catania; ItaliaFil: Pian, Elena. Osservatorio Astronomico di Trieste; ItaliaFil: Sollerman, Jesper. The Oskar Klein Centre; SueciaFil: Benetti, Stefano. Osservatorio Astronomico di Padova; ItaliaFil: Pignata, Giuliano. Universidad Andres Bello; ChileFil: Valenti, Stefano. Osservatorio Astronomico di Padova; ItaliaFil: Covino, Stefano. Osservatorio Astronomico di Brera; ItaliaFil: D´Avanzo, Paolo. Osservatorio Astronomico di Brera; ItaliaFil: Malesani, Daniele. University of Copenhagen; DinamarcaFil: Cappellaro, Enrico. Osservatorio Astronomico di Padova; ItaliaFil: Della Valle, Massimo. Osservatorio Astronomico di Capodimonte; ItaliaFil: Fynbo, Johan. Universidad de Copenhagen; DinamarcaFil: Hjorth, Jens. Universidad de Copenhagen; DinamarcaFil: Mazzali, Paolo, A.. Osservatorio Astronomico di Padova; ItaliaFil: Reichart, Daniel E.. University of North Carolina; Estados UnidosFil: Starling, Rhaana L. C.. University of Leicester; Reino UnidoFil: Turatto, Massimo. Osservatorio Astronomico di Trieste; ItaliaFil: Vergani, Susanna D.. Osservatorio Astronomico di Brera; ItaliaFil: Wiersema, Klass. University of Leicester; Reino UnidoFil: Amati, Lorenzo. Istituto di Astrofisica Spaziale e Fisica cosmica; ItaliaFil: Bersier, David. Liverpool John Moores University; Reino UnidoFil: Campana, Sergio. Osservatorio Astronomico di Brera; ItaliaFil: Cano, Zach. Liverpool John Moores University; Reino UnidoFil: Castro Tirado, Alberto J.. Instituto de Astrofisica de Andalucia; EspañaFil: Chincarini, Guido. Univerisit Milano Bicocca; ItaliaFil: D´Elia, Valerio. Osservatorio Astronomico di Roma; ItaliaFil: de Ugarte Postigo, Antonio. Universidad de Copenhagen; DinamarcaFil: Deng, Jinsong. National Astronomical Observatories; ChinaFil: Ferrero, Patricia. Instituto de Astrofsica de Canarias; EspañaFil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaIOP Publishing2012-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdftext/richtextapplication/pdfhttp://hdl.handle.net/11336/21217Bufano, Filomena; Pian, Elena; Sollerman, Jesper; Benetti, Stefano; Pignata, Giuliano; et al.; The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D; IOP Publishing; Astrophysical Journal; 753; 1; 7-2012; 67-790004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/pdf/1111.4527.pdfinfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/753/1/67info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:40:01Zoai:ri.conicet.gov.ar:11336/21217instacron: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 10:40:02.064CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| title |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| spellingShingle |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D Bufano, Filomena supernovae: general supernovae: individual: SN 2010bh GRB 100316D |
| title_short |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| title_full |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| title_fullStr |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| title_full_unstemmed |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| title_sort |
The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D |
| dc.creator.none.fl_str_mv |
Bufano, Filomena Pian, Elena Sollerman, Jesper Benetti, Stefano Pignata, Giuliano Valenti, Stefano Covino, Stefano D´Avanzo, Paolo Malesani, Daniele Cappellaro, Enrico Della Valle, Massimo Fynbo, Johan Hjorth, Jens Mazzali, Paolo, A. Reichart, Daniel E. Starling, Rhaana L. C. Turatto, Massimo Vergani, Susanna D. Wiersema, Klass Amati, Lorenzo Bersier, David Campana, Sergio Cano, Zach Castro Tirado, Alberto J. Chincarini, Guido D´Elia, Valerio de Ugarte Postigo, Antonio Deng, Jinsong Ferrero, Patricia Mirabel Miquele, Igor Felix |
| author |
Bufano, Filomena |
| author_facet |
Bufano, Filomena Pian, Elena Sollerman, Jesper Benetti, Stefano Pignata, Giuliano Valenti, Stefano Covino, Stefano D´Avanzo, Paolo Malesani, Daniele Cappellaro, Enrico Della Valle, Massimo Fynbo, Johan Hjorth, Jens Mazzali, Paolo, A. Reichart, Daniel E. Starling, Rhaana L. C. Turatto, Massimo Vergani, Susanna D. Wiersema, Klass Amati, Lorenzo Bersier, David Campana, Sergio Cano, Zach Castro Tirado, Alberto J. Chincarini, Guido D´Elia, Valerio de Ugarte Postigo, Antonio Deng, Jinsong Ferrero, Patricia Mirabel Miquele, Igor Felix |
| author_role |
author |
| author2 |
Pian, Elena Sollerman, Jesper Benetti, Stefano Pignata, Giuliano Valenti, Stefano Covino, Stefano D´Avanzo, Paolo Malesani, Daniele Cappellaro, Enrico Della Valle, Massimo Fynbo, Johan Hjorth, Jens Mazzali, Paolo, A. Reichart, Daniel E. Starling, Rhaana L. C. Turatto, Massimo Vergani, Susanna D. Wiersema, Klass Amati, Lorenzo Bersier, David Campana, Sergio Cano, Zach Castro Tirado, Alberto J. Chincarini, Guido D´Elia, Valerio de Ugarte Postigo, Antonio Deng, Jinsong Ferrero, Patricia Mirabel Miquele, Igor Felix |
| 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 author author author author author author |
| dc.subject.none.fl_str_mv |
supernovae: general supernovae: individual: SN 2010bh GRB 100316D |
| topic |
supernovae: general supernovae: individual: SN 2010bh GRB 100316D |
| 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 spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed Type Ic supernova, SN 2010bh, associated with the soft, long-duration gamma-ray burst (X-ray flash) GRB 100316D. Intensive follow-up observations of SN 2010bh were performed at the ESO Very Large Telescope (VLT) using the X-shooter and FORS2 instruments. Thanks to the detailed temporal coverage and the extended wavelength range (3000-24800 Å), we obtained an unprecedentedly rich spectral sequence among the hypernovae, making SN 2010bh one of the best studied representatives of this SN class. We find that SN 2010bh has a more rapid rise to maximum brightness (8.0 ± 1.0 rest-frame days) and a fainter absolute peak luminosity (L bol ≈ 3 × 1042 erg s–1) than previously observed SN events associated with GRBs. Our estimate of the ejected 56Ni mass is 0.12 ± 0.02 M ☉. From the broad spectral features, we measure expansion velocities up to 47,000 km s–1, higher than those of SNe 1998bw (GRB 980425) and 2006aj (GRB 060218). Helium absorption lines He I λ5876 and He I 1.083 μm, blueshifted by ~20,000-30,000 km s–1 and ~28,000-38,000 km s–1, respectively, may be present in the optical spectra. However, the lack of coverage of the He I 2.058 μm line prevents us from confirming such identifications. The nebular spectrum, taken at ~186 days after the explosion, shows a broad but faint [O I] emission at 6340 Å. The light curve shape and photospheric expansion velocities of SN 2010bh suggest that we witnessed a highly energetic explosion with a small ejected mass (E k ≈ 1052 erg and M ej ≈ 3 M ☉). The observed properties of SN 2010bh further extend the heterogeneity of the class of GRB SNe. Fil: Bufano, Filomena. Osservatorio Astronomico di Catania; Italia Fil: Pian, Elena. Osservatorio Astronomico di Trieste; Italia Fil: Sollerman, Jesper. The Oskar Klein Centre; Suecia Fil: Benetti, Stefano. Osservatorio Astronomico di Padova; Italia Fil: Pignata, Giuliano. Universidad Andres Bello; Chile Fil: Valenti, Stefano. Osservatorio Astronomico di Padova; Italia Fil: Covino, Stefano. Osservatorio Astronomico di Brera; Italia Fil: D´Avanzo, Paolo. Osservatorio Astronomico di Brera; Italia Fil: Malesani, Daniele. University of Copenhagen; Dinamarca Fil: Cappellaro, Enrico. Osservatorio Astronomico di Padova; Italia Fil: Della Valle, Massimo. Osservatorio Astronomico di Capodimonte; Italia Fil: Fynbo, Johan. Universidad de Copenhagen; Dinamarca Fil: Hjorth, Jens. Universidad de Copenhagen; Dinamarca Fil: Mazzali, Paolo, A.. Osservatorio Astronomico di Padova; Italia Fil: Reichart, Daniel E.. University of North Carolina; Estados Unidos Fil: Starling, Rhaana L. C.. University of Leicester; Reino Unido Fil: Turatto, Massimo. Osservatorio Astronomico di Trieste; Italia Fil: Vergani, Susanna D.. Osservatorio Astronomico di Brera; Italia Fil: Wiersema, Klass. University of Leicester; Reino Unido Fil: Amati, Lorenzo. Istituto di Astrofisica Spaziale e Fisica cosmica; Italia Fil: Bersier, David. Liverpool John Moores University; Reino Unido Fil: Campana, Sergio. Osservatorio Astronomico di Brera; Italia Fil: Cano, Zach. Liverpool John Moores University; Reino Unido Fil: Castro Tirado, Alberto J.. Instituto de Astrofisica de Andalucia; España Fil: Chincarini, Guido. Univerisit Milano Bicocca; Italia Fil: D´Elia, Valerio. Osservatorio Astronomico di Roma; Italia Fil: de Ugarte Postigo, Antonio. Universidad de Copenhagen; Dinamarca Fil: Deng, Jinsong. National Astronomical Observatories; China Fil: Ferrero, Patricia. Instituto de Astrofsica de Canarias; España Fil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina |
| description |
We present the spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed Type Ic supernova, SN 2010bh, associated with the soft, long-duration gamma-ray burst (X-ray flash) GRB 100316D. Intensive follow-up observations of SN 2010bh were performed at the ESO Very Large Telescope (VLT) using the X-shooter and FORS2 instruments. Thanks to the detailed temporal coverage and the extended wavelength range (3000-24800 Å), we obtained an unprecedentedly rich spectral sequence among the hypernovae, making SN 2010bh one of the best studied representatives of this SN class. We find that SN 2010bh has a more rapid rise to maximum brightness (8.0 ± 1.0 rest-frame days) and a fainter absolute peak luminosity (L bol ≈ 3 × 1042 erg s–1) than previously observed SN events associated with GRBs. Our estimate of the ejected 56Ni mass is 0.12 ± 0.02 M ☉. From the broad spectral features, we measure expansion velocities up to 47,000 km s–1, higher than those of SNe 1998bw (GRB 980425) and 2006aj (GRB 060218). Helium absorption lines He I λ5876 and He I 1.083 μm, blueshifted by ~20,000-30,000 km s–1 and ~28,000-38,000 km s–1, respectively, may be present in the optical spectra. However, the lack of coverage of the He I 2.058 μm line prevents us from confirming such identifications. The nebular spectrum, taken at ~186 days after the explosion, shows a broad but faint [O I] emission at 6340 Å. The light curve shape and photospheric expansion velocities of SN 2010bh suggest that we witnessed a highly energetic explosion with a small ejected mass (E k ≈ 1052 erg and M ej ≈ 3 M ☉). The observed properties of SN 2010bh further extend the heterogeneity of the class of GRB SNe. |
| publishDate |
2012 |
| dc.date.none.fl_str_mv |
2012-07 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
| status_str |
publishedVersion |
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http://hdl.handle.net/11336/21217 Bufano, Filomena; Pian, Elena; Sollerman, Jesper; Benetti, Stefano; Pignata, Giuliano; et al.; The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D; IOP Publishing; Astrophysical Journal; 753; 1; 7-2012; 67-79 0004-637X CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/21217 |
| identifier_str_mv |
Bufano, Filomena; Pian, Elena; Sollerman, Jesper; Benetti, Stefano; Pignata, Giuliano; et al.; The Highly Energetic Expansion of SN 2010bh Associated with GRB 100316D; IOP Publishing; Astrophysical Journal; 753; 1; 7-2012; 67-79 0004-637X CONICET Digital CONICET |
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eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/pdf/1111.4527.pdf info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/753/1/67 |
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