Mostrar el registro sencillo del ítem
dc.contributor.author
Butt, Yousaf M.
dc.contributor.author
Torres, Diego F.
dc.contributor.author
Combi, Jorge Ariel
dc.contributor.author
Dame, Thomas M.
dc.contributor.author
Romero, Gustavo Esteban
dc.date.available
2017-12-28T16:13:05Z
dc.date.issued
2001-12
dc.identifier.citation
Butt, Yousaf M.; Torres, Diego F.; Combi, Jorge Ariel; Dame, Thomas M.; Romero, Gustavo Esteban; Is the supernova remnant RX J1713.7-3946 a hadronic cosmic-ray accelerator?; IOP Publishing; Astrophysical Journal; 562; 2; 12-2001; L167-L171
dc.identifier.issn
0004-637X
dc.identifier.uri
http://hdl.handle.net/11336/31804
dc.description.abstract
The nonthermal supernova remnant (SNR) RX J1713.7-3946 has recently been shown to be a site of cosmic-ray (CR) electron acceleration to TeV energies. Here we present evidence that this remnant is also accelerating CR nuclei. Such energetic nuclei can interact with ambient interstellar gas to produce high-energy gamma rays via the decay of neutral pions. We associate the unidentified EGRET GeV gamma-ray source, 3EG J1714-3857, with a very massive (~3×105 Msolar) and dense (~500 nucleons cm-3) molecular cloud interacting with SNR RX J1713.7-3946. Direct evidence for such interaction is provided by observations of the lowest two rotational transitions of CO molecules in the cloud; as in other clear cases of interaction, the CO(J=2-->1)/CO(J=1-->0) ratio is significantly enhanced. Since the cloud is of low radio and X-ray brightness, electrons cannot be responsible for the bulk of the GeV emission there. A picture thus emerges in which both electrons and nuclei are being accelerated by the SNR: whereas the relativistic electrons dominate the local nonthermal radio, X-ray, and TeV emission, the shock-accelerated CR protons and ions (hadrons) are exposed through their interactions in the adjacent massive cloud, leading to the observed GeV emission via the gamma decay of neutral pions.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
IOP Publishing
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by/2.5/ar/
dc.subject
Acceleration of Particles
dc.subject
Cosmic Rays
dc.subject
Interstellar Clouds
dc.subject
Supernova Remnants
dc.subject.classification
Astronomía
dc.subject.classification
Ciencias Físicas
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
dc.title
Is the supernova remnant RX J1713.7-3946 a hadronic cosmic-ray accelerator?
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2017-11-24T13:48:24Z
dc.journal.volume
562
dc.journal.number
2
dc.journal.pagination
L167-L171
dc.journal.pais
Reino Unido
dc.journal.ciudad
Londres
dc.description.fil
Fil: Butt, Yousaf M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
dc.description.fil
Fil: Torres, Diego F.. University of Princeton; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
dc.description.fil
Fil: Combi, Jorge Ariel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
dc.description.fil
Fil: Dame, Thomas M.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
dc.description.fil
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
dc.journal.title
Astrophysical Journal
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1086/324592
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/324592/meta
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0109292
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://core.ac.uk/reader/159301356
Archivos asociados