The production of orbitally modulated UHE photons in LS 5039
[Conntext] Gamma-ray binaries present emission that is variable and can reach ultra-high energies. The processes behind the acceleration of the particles that produce this very energetic radiation are yet to be understood.
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/402719 |
| Acceso en línea: | http://hdl.handle.net/10261/402719 https://api.elsevier.com/content/abstract/scopus_id/105013202630 |
| Access Level: | acceso abierto |
| Palabra clave: | Acceleration of particles Gamma rays: stars Radiation mechanisms: non-thermal Stars: winds, outflows X-rays: binaries |
| Sumario: | [Conntext] Gamma-ray binaries present emission that is variable and can reach ultra-high energies. The processes behind the acceleration of the particles that produce this very energetic radiation are yet to be understood. |
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