Heavy nuclei at the end of the cosmic ray spectrum
- Autores
- Anchordoqui, Luis Alfredo; Romero, Gustavo Esteban; Combi, Jorge Ariel
- Año de publicación
- 1999
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We provide an account of the possible acceleration of iron nuclei up to energies 300 EeV in the nearby, metally rich starburst galaxy NGC 253. It is suggested that particles can escape from the nuclear region with energies of ~1015 eV and can then be reaccelerated at the terminal shock of the galactic superwind generated by the starburst, avoiding the photodisintegration expected if the nuclei were accelerated in the central region of high photon density. We have also made estimates of the expected arrival spectrum, which displays a strong dependence on the energy cutoff at the source.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
Cosmic ray
Physics
Spectrum (functional analysis)
Energy (signal processing)
Photodisintegration
Photon density
Central region
Astrophysics
Galaxy - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/122767
Ver los metadatos del registro completo
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Heavy nuclei at the end of the cosmic ray spectrumAnchordoqui, Luis AlfredoRomero, Gustavo EstebanCombi, Jorge ArielCiencias AstronómicasCosmic rayPhysicsSpectrum (functional analysis)Energy (signal processing)PhotodisintegrationPhoton densityCentral regionAstrophysicsGalaxyWe provide an account of the possible acceleration of iron nuclei up to energies 300 EeV in the nearby, metally rich starburst galaxy NGC 253. It is suggested that particles can escape from the nuclear region with energies of ~10<sup>15</sup> eV and can then be reaccelerated at the terminal shock of the galactic superwind generated by the starburst, avoiding the photodisintegration expected if the nuclei were accelerated in the central region of high photon density. We have also made estimates of the expected arrival spectrum, which displays a strong dependence on the energy cutoff at the source.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía1999-10-25info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/122767enginfo:eu-repo/semantics/altIdentifier/issn/0556-2821info:eu-repo/semantics/altIdentifier/issn/1089-4918info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/9903145info:eu-repo/semantics/altIdentifier/doi/10.1103/physrevd.60.103001info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:29:14Zoai:sedici.unlp.edu.ar:10915/122767Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:29:15.008SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Heavy nuclei at the end of the cosmic ray spectrum |
title |
Heavy nuclei at the end of the cosmic ray spectrum |
spellingShingle |
Heavy nuclei at the end of the cosmic ray spectrum Anchordoqui, Luis Alfredo Ciencias Astronómicas Cosmic ray Physics Spectrum (functional analysis) Energy (signal processing) Photodisintegration Photon density Central region Astrophysics Galaxy |
title_short |
Heavy nuclei at the end of the cosmic ray spectrum |
title_full |
Heavy nuclei at the end of the cosmic ray spectrum |
title_fullStr |
Heavy nuclei at the end of the cosmic ray spectrum |
title_full_unstemmed |
Heavy nuclei at the end of the cosmic ray spectrum |
title_sort |
Heavy nuclei at the end of the cosmic ray spectrum |
dc.creator.none.fl_str_mv |
Anchordoqui, Luis Alfredo Romero, Gustavo Esteban Combi, Jorge Ariel |
author |
Anchordoqui, Luis Alfredo |
author_facet |
Anchordoqui, Luis Alfredo Romero, Gustavo Esteban Combi, Jorge Ariel |
author_role |
author |
author2 |
Romero, Gustavo Esteban Combi, Jorge Ariel |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Cosmic ray Physics Spectrum (functional analysis) Energy (signal processing) Photodisintegration Photon density Central region Astrophysics Galaxy |
topic |
Ciencias Astronómicas Cosmic ray Physics Spectrum (functional analysis) Energy (signal processing) Photodisintegration Photon density Central region Astrophysics Galaxy |
dc.description.none.fl_txt_mv |
We provide an account of the possible acceleration of iron nuclei up to energies 300 EeV in the nearby, metally rich starburst galaxy NGC 253. It is suggested that particles can escape from the nuclear region with energies of ~10<sup>15</sup> eV and can then be reaccelerated at the terminal shock of the galactic superwind generated by the starburst, avoiding the photodisintegration expected if the nuclei were accelerated in the central region of high photon density. We have also made estimates of the expected arrival spectrum, which displays a strong dependence on the energy cutoff at the source. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
description |
We provide an account of the possible acceleration of iron nuclei up to energies 300 EeV in the nearby, metally rich starburst galaxy NGC 253. It is suggested that particles can escape from the nuclear region with energies of ~10<sup>15</sup> eV and can then be reaccelerated at the terminal shock of the galactic superwind generated by the starburst, avoiding the photodisintegration expected if the nuclei were accelerated in the central region of high photon density. We have also made estimates of the expected arrival spectrum, which displays a strong dependence on the energy cutoff at the source. |
publishDate |
1999 |
dc.date.none.fl_str_mv |
1999-10-25 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/122767 |
url |
http://sedici.unlp.edu.ar/handle/10915/122767 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0556-2821 info:eu-repo/semantics/altIdentifier/issn/1089-4918 info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/9903145 info:eu-repo/semantics/altIdentifier/doi/10.1103/physrevd.60.103001 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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