Double degenerate mergers as progenitors of high-field magnetic white dwarfs
High-field magnetic white dwarfs have been long suspected to be the result of stellar mergers. However, the nature of the coalescing stars and the precise mechanism that produces the magnetic field are still unknown. Here, we show that the hot, convective, differentially rotating corona present in t...
Guardado en:
| Autores principales: | García Berro, Enrique, Lorén Aguilar, Pablo, Aznar Siguán, Gabriela, Torres, Santiago, Camacho, Judit, Althaus, Leandro Gabriel, Córsico, Alejandro Hugo, Külebi, Baybars, Isern, Jordi |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93578 http://iopscience.iop.org/article/10.1088/0004-637X/749/1/25/meta https://ri.conicet.gov.ar/handle/11336/42642 |
| Aporte de: |
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