Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Universidad Nacional de Río Negro | - |
| dc.creator | Romero, Gustavo E. | - |
| dc.creator | Christiansen, Hugo | - |
| dc.creator | Orellana, Mariana D. | - |
| dc.date | 2005-10-20 | - |
| dc.date.accessioned | 2020-02-11T14:09:27Z | - |
| dc.date.available | 2020-02-11T14:09:27Z | - |
| dc.date.issued | 2005-10-20 | - |
| dc.identifier | Romero, Gustavo E., Christiansen, Hugo. & Orellana, Mariana D. (2005). Hadronic high-energy gamma ray emission from microquasars. IOP Publishing; Astrophysical Journal; 632; 1093-1098 | - |
| dc.identifier | 0004-637X | - |
| dc.identifier | http://dx.doi.org/10.1086/444446 | - |
| dc.identifier | http://adsabs.harvard.edu/abs/2005ApJ...632.1093R | - |
| dc.identifier | http://hdl.handle.net/11336/29928 | - |
| dc.identifier | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2824 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar/jspui/handle/bnmm/575883 | - |
| dc.description | Fil: Romero, Gustavo E. Comisión de Investigaciones Científicas; Argentina | - |
| dc.description | Fil: Romero, Gustavo E. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina | - |
| dc.description | Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomía; Argentina | - |
| dc.description | Fil: Christiansen, Hugo. Universidade Estadual Do Ceara; Brasil | - |
| dc.description | Fil: Orellana, Mariana D. Universidad Nacional de Río Negro; Argentina | - |
| dc.description | Fil: Orellana, Mariana D. Comisión de Investigaciones Científicas; Argentina | - |
| dc.description | Fil: Orellana, Mariana D. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina | - |
| dc.description | Fil: Orellana, Mariana D. Instituto Argentino de Radioastronomía; Argentina | - |
| dc.description | We present a hadronic model for gamma-ray production in the microquasar LS I +61 303. The system is formed by a neutron star that accretes matter from the dense and slow equatorial wind of the Be primary star. We calculate the gamma-ray emission originating from pp interactions between relativistic protons in the jet and cold protons from the wind. After taking into account opacity effects on the gamma rays introduced by the different photon fields, we present high-energy spectral predictions that can be tested with the new-generation Cerenkov telescope MAGIC. | - |
| dc.format | application/pdf | - |
| dc.language | spa | - |
| dc.relation | 632 | - |
| dc.relation | Astrophysical Journal | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/4.0/ | - |
| dc.source | reponame:RID-UNRN (UNRN) | - |
| dc.source | instname:Universidad Nacional de Río Negro | - |
| dc.source | instacron:UNRN | - |
| dc.source.uri | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2824 | - |
| dc.subject | Gamma rays | - |
| dc.subject | Hadrons | - |
| dc.subject | Microquasars | - |
| dc.subject | .::Ciencias Exactas y Naturales | - |
| dc.title | Hadronic high-energy gamma ray emission from microquasars | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/acceptedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| dc.about | - | |
| Aparece en las colecciones: | Universidad Nacional de Río Negro | |
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