A population synthesis study of the Gaia 100 pc unresolved white dwarf-main sequence binary population
[Context] Binaries consisting of a white dwarf and a main-sequence star (WDMSs) are excellent tools for studying a wide variety of open problems in modern astronomy. However, due to selection effects, the currently known WDMS population is severely affected by observational biases. This is particula...
| 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:10261/399118 |
| Acceso en línea: | http://hdl.handle.net/10261/399118 http://arxiv.org/abs/2502.11593v1 |
| Access Level: | acceso abierto |
| Palabra clave: | Binaries: close Binaries: eclipsing Binaries: general White dwarfs |
| Sumario: | [Context] Binaries consisting of a white dwarf and a main-sequence star (WDMSs) are excellent tools for studying a wide variety of open problems in modern astronomy. However, due to selection effects, the currently known WDMS population is severely affected by observational biases. This is particularly the case for unresolved systems in which the main-sequence companions usually outshine the white dwarf components. |
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