Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.provenance | Universidad Nacional de Río Negro | - |
| dc.creator | Romero, Gustavo E. | - |
| dc.creator | Orellana, Mariana D. | - |
| dc.creator | Okazaki, A. | - |
| dc.creator | Owocki, S. | - |
| dc.date | 2008-09 | - |
| dc.date.accessioned | 2020-02-11T14:09:29Z | - |
| dc.date.available | 2020-02-11T14:09:29Z | - |
| dc.date.issued | 2008-09 | - |
| dc.identifier | Romero, Gustavo E., Orellana, Mariana D., Okazaki, A. & Owocki, S. (2008). LS I+61 303: microquasar or not microquasar?. World Scientific; International Journal of Modern Physics D; 17; 10; 1875-1881 | - |
| dc.identifier | 0218-2718 | - |
| dc.identifier | http://www.worldscientific.com/doi/abs/10.1142/S0218271808013510 | - |
| dc.identifier | http://hdl.handle.net/11336/27815 | - |
| dc.identifier | https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2828 | - |
| dc.identifier | http://dx.doi.org/10.1142/S0218271808013510 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar/jspui/handle/bnmm/575888 | - |
| dc.description | Fil: Romero, Gustavo E. Instituto Argentino de Radioastronomia; 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. Comisión de Investigaciones Científicas; Argentina | - |
| dc.description | Fil: Orellana, Mariana D. Instituto Argentino de Radioastronomia; 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. Comisión de Investigaciones Científicas; Argentina | - |
| dc.description | Fil: Okazaki, A. Hokkai-Gakuen University; Japón | - |
| dc.description | Fil: Owocki, S. University of Delaware; Estados Unidos | - |
| dc.description | LS I +61 303 is a puzzling object detected from radio up to high-energy gamma-rays. Variability has recently been observed in its high-energy emission. The object is a binary system, with a compact object and a Be star as primary. The nature of the secondary and the origin of the gamma-ray emission are not clearly established at present. Recent VLBA radio data have been used to claim that the system is a Be/neutron star colliding wind binary, instead of a microquasar. We review the main views on the nature of LS I +61 303 and present results of 3D SPH simulations that can shed some light on the nature of the system. Our results support an accretion powered source, compatible with a microquasar interpretation. | - |
| dc.format | application/pdf | - |
| dc.language | spa | - |
| dc.relation | 17 | - |
| dc.relation | International Journal of Modern Physics D | - |
| 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 | http://dx.doi.org/10.1142/S0218271808013510 | - |
| dc.subject | X Ray Binaries | - |
| dc.subject | Gamma Rays | - |
| dc.subject | LS I +61 303 (estrella) | - |
| dc.subject | .::Ciencias Exactas y Naturales::Ciencias Físicas | - |
| dc.title | LS I+61 303: microquasar or not microquasar? | - |
| 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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