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dc.contributor | Universitat Politècnica de Catalunya. Departament de Física Aplicada |
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dc.contributor | Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica |
dc.contributor | Universitat Politècnica de Catalunya. CTE-CRAE - Grup de Recerca en Ciències i Tecnologies de l'Espai |
dc.contributor.author | García-Berro Montilla, Enrique |
dc.contributor.author | Torres Gil, Santiago |
dc.contributor.author | Lorén Aguilar, Pablo |
dc.contributor.author | Aznar Siguan, Gabriela |
dc.contributor.author | Camacho Díaz, Judit |
dc.contributor.author | Kulebi, Baybar |
dc.contributor.author | Isern Vilaboy, Jordi |
dc.contributor.author | Althaus, Leandro Gabriel |
dc.contributor.author | Corsico, Alejandro H. |
dc.date | 2013-01-01 |
dc.identifier.citation | Garcia-berro, E. [et al.]. On the origin of high-field magnetic white dwarfs. A: "18th European White Dwarf Workshop. Astronomical Society of the Pacific Conference Series". 390 ASHTON AVE. SAN FRANCISCO: Astronomical Society of the Pacific, 2013, p. 423-428. |
dc.identifier.citation | 978-1-58381-820-6 |
dc.identifier.uri | http://hdl.handle.net/2117/24432 |
dc.language.iso | eng |
dc.publisher | Astronomical Society of the Pacific |
dc.relation | http://aspbooks.org/custom/publications/paper/469-0423.html |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Spain |
dc.rights | info:eu-repo/semantics/openAccess |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ |
dc.subject | Àrees temàtiques de la UPC::Física::Astronomia i astrofísica |
dc.subject | White dwarf stars |
dc.subject | High-field magnetic white dwarfs have been long suspected to be the result of stellar mergers. However |
dc.subject | the nature of the coalescing stars and the precise mechanism that produces the magnetic field are still unknown. Here we show that the hot |
dc.subject | convective |
dc.subject | differentially rotating corona present in the outer layers of the remnant of the merger of two degenerate cores is able to produce magnetic fields of the required strength that do not decay for long timescales. We also show |
dc.subject | using an state-of-the-art Monte Carlo simulator |
dc.subject | that the expected number of high-field magnetic white dwarfs produced in this way is consistent with that found in the solar neighborhood. |
dc.subject | Estels nans |
dc.title | On the origin of high-field magnetic white dwarfs |
dc.type | info:eu-repo/semantics/publishedVersion |
dc.type | info:eu-repo/semantics/conferenceObject |
dc.description.abstract | |
dc.description.abstract |