Semi-analytic studies of the accretion disk and magnetic field geometry in M 87*
Context. Magnetic fields play a pivotal role in the dynamics of black hole accretion flows and in the formation of relativistic jets. Observations by the Event Horizon Telescope (EHT) provided unprecedented insights into accretion structures near black holes. Interpreting these observations requires...
| Autores: | , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2026 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:dnet:digitalcsic_::d40a5f7b0233ae52686012eeb7fa7622 |
| Acceso en línea: | http://hdl.handle.net/10261/427917 |
| Access Level: | acceso abierto |
| Palabra clave: | Accretion, accretion disks Black hole physics Gravitation Magnetic fields Polarization Radiative transfer |
| Sumario: | Context. Magnetic fields play a pivotal role in the dynamics of black hole accretion flows and in the formation of relativistic jets. Observations by the Event Horizon Telescope (EHT) provided unprecedented insights into accretion structures near black holes. Interpreting these observations requires a theoretical framework that links polarized emission to the underlying system properties and magnetic field geometries. |
|---|