Hydrodynamic simulations of the recurrent nova T Coronae Borealis: Nucleosynthesis predictions
[Context] Recurrent novae are, by definition, novae observed in outburst more than once or identified by the presence of vast super-shells, ejected in previous eruptions, surrounding the system. These systems are characterized by remarkably short recurrence times between outbursts, typically ranging...
| 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:10261/398410 |
| Acceso en línea: | http://hdl.handle.net/10261/398410 |
| Access Level: | acceso abierto |
| Palabra clave: | Hydrodynamics Nuclear reactions, nucleosynthesis, abundances Binaries: close Novae, cataclysmic variable |
| Sumario: | [Context] Recurrent novae are, by definition, novae observed in outburst more than once or identified by the presence of vast super-shells, ejected in previous eruptions, surrounding the system. These systems are characterized by remarkably short recurrence times between outbursts, typically ranging from 1 to about 100 yr. Such short recurrence times require very high mass-accretion rates, white dwarf masses approaching the Chandrasekhar limit, and very high initial white dwarf luminosities. |
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