Supersoft luminous X-ray sources in galactic nuclei
[Context] Tidal disruption events (TDEs) are usually discovered at X-ray or optical wavelengths through their transient nature. A characteristic spectral feature of X-ray detected TDEs is a ‘supersoft’ X-ray emission, not observed in any other extragalactic source, with the exception of a few rapidl...
| Autores: | , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/336025 |
| Acceso en línea: | http://hdl.handle.net/10261/336025 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: nuclei X-rays: galaxies Galaxies: active |
| Sumario: | [Context] Tidal disruption events (TDEs) are usually discovered at X-ray or optical wavelengths through their transient nature. A characteristic spectral feature of X-ray detected TDEs is a ‘supersoft’ X-ray emission, not observed in any other extragalactic source, with the exception of a few rapidly variable hyperluminous X-ray sources (HLXs) or supersoft active galactic nuclei (AGN) that are distinguishable by their optical emission. |
|---|