Strange-pulsar evolution and soft γ-repeaters
- Autores
- Horvath, Jorge Ernesto; Vucetich, Héctor; Benvenuto, Omar Gustavo
- Año de publicación
- 1993
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Soft γ-repeaters are puzzling sources which produce γ-transients, and which have been tentatively identified as a separate subclass from sources which produce «classical» γ-bursts. We sketch the features of a model for soft γ-repeaters based on the evolutionary history of strange pulsars. It is shown that the main features of soft γ-repeaters can be explained by strange-pulsar evolution
Facultad de Ciencias Exactas
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Física
Astronomía
dense matter
elementary particles
stars: peculiar
pulsars: general
gamma-rays: bursts - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/140310
Ver los metadatos del registro completo
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Strange-pulsar evolution and soft γ-repeatersHorvath, Jorge ErnestoVucetich, HéctorBenvenuto, Omar GustavoFísicaAstronomíadense matterelementary particlesstars: peculiarpulsars: generalgamma-rays: burstsSoft γ-repeaters are puzzling sources which produce γ-transients, and which have been tentatively identified as a separate subclass from sources which produce «classical» γ-bursts. We sketch the features of a model for soft γ-repeaters based on the evolutionary history of strange pulsars. It is shown that the main features of soft γ-repeaters can be explained by strange-pulsar evolutionFacultad de Ciencias ExactasFacultad de Ciencias Astronómicas y Geofísicas1993info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf506-510http://sedici.unlp.edu.ar/handle/10915/140310enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/issn/1365-2966info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/262.2.506info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-11-12T10:56:09Zoai:sedici.unlp.edu.ar:10915/140310Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-11-12 10:56:10.021SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Strange-pulsar evolution and soft γ-repeaters |
| title |
Strange-pulsar evolution and soft γ-repeaters |
| spellingShingle |
Strange-pulsar evolution and soft γ-repeaters Horvath, Jorge Ernesto Física Astronomía dense matter elementary particles stars: peculiar pulsars: general gamma-rays: bursts |
| title_short |
Strange-pulsar evolution and soft γ-repeaters |
| title_full |
Strange-pulsar evolution and soft γ-repeaters |
| title_fullStr |
Strange-pulsar evolution and soft γ-repeaters |
| title_full_unstemmed |
Strange-pulsar evolution and soft γ-repeaters |
| title_sort |
Strange-pulsar evolution and soft γ-repeaters |
| dc.creator.none.fl_str_mv |
Horvath, Jorge Ernesto Vucetich, Héctor Benvenuto, Omar Gustavo |
| author |
Horvath, Jorge Ernesto |
| author_facet |
Horvath, Jorge Ernesto Vucetich, Héctor Benvenuto, Omar Gustavo |
| author_role |
author |
| author2 |
Vucetich, Héctor Benvenuto, Omar Gustavo |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Física Astronomía dense matter elementary particles stars: peculiar pulsars: general gamma-rays: bursts |
| topic |
Física Astronomía dense matter elementary particles stars: peculiar pulsars: general gamma-rays: bursts |
| dc.description.none.fl_txt_mv |
Soft γ-repeaters are puzzling sources which produce γ-transients, and which have been tentatively identified as a separate subclass from sources which produce «classical» γ-bursts. We sketch the features of a model for soft γ-repeaters based on the evolutionary history of strange pulsars. It is shown that the main features of soft γ-repeaters can be explained by strange-pulsar evolution Facultad de Ciencias Exactas Facultad de Ciencias Astronómicas y Geofísicas |
| description |
Soft γ-repeaters are puzzling sources which produce γ-transients, and which have been tentatively identified as a separate subclass from sources which produce «classical» γ-bursts. We sketch the features of a model for soft γ-repeaters based on the evolutionary history of strange pulsars. It is shown that the main features of soft γ-repeaters can be explained by strange-pulsar evolution |
| publishDate |
1993 |
| dc.date.none.fl_str_mv |
1993 |
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eng |
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eng |
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