Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Araudo, Anabella Teresa | - |
| dc.creator | Bosch Ramon, Valentí | - |
| dc.creator | Romero, Gustavo Esteban | - |
| dc.date | 2017-05-22T21:23:28Z | - |
| dc.date | 2017-05-22T21:23:28Z | - |
| dc.date | 2013-10 | - |
| dc.date | 2017-05-15T17:05:25Z | - |
| dc.date.accessioned | 2019-04-29T15:54:15Z | - |
| dc.date.available | 2019-04-29T15:54:15Z | - |
| dc.date.issued | 2013-10 | - |
| dc.identifier | Araudo, Anabella Teresa; Bosch Ramon, Valentí; Romero, Gustavo Esteban; Gamma-ray emission from massive stars interacting with active galactic nuclei jets; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 436; 10-2013; 3626-3639 | - |
| dc.identifier | 0035-8711 | - |
| dc.identifier | http://hdl.handle.net/11336/16839 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/305080 | - |
| dc.description | Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by the supermassive black hole. In this work, we study the interaction of early-type stars with relativistic jets in active galactic nuclei. A bow-shaped double-shock structure is formed as a consequence of the interaction of the jet and the stellar wind of each early-type star. Particles can be accelerated up to relativistic energies in these shocks and emit high-energy radiation. We compute, considering different stellar densities of the galactic core, the gamma-ray emission produced by non-thermal radiative processes. This radiation may be significant in some cases, and its detection might yield valuable information on the properties of the stellar population in the galaxy nucleus, as well as on the relativistic jet. This emission is expected to be particularly relevant for nearby non-blazar sources. | - |
| dc.description | Fil: Araudo, Anabella Teresa. Universidad Nacional Autónoma de México; México | - |
| dc.description | Fil: Bosch Ramon, Valentí. Universidad de Barcelona; España | - |
| dc.description | Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comision de Invest.científicas. Instituto Argentino de Radioastronomia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - la Plata. Instituto Argentino de Radioastronomia; Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Oxford University Press | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stt1840 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stt1840 | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | Radiation mechanisms | - |
| dc.subject | Early type stars | - |
| dc.subject | Active galaxies | - |
| dc.subject | Gamma rays | - |
| dc.subject | Non thermal mechanisms | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Gamma-ray emission from massive stars interacting with active galactic nuclei jets | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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