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Magnetic white dwarfs with debris discs

Autor
Kulebi, B.; Eksi, K.Y.; Loren, P.; Garcia-berro, E.; Isern, J.
Tipus d'activitat
Article en revista
Revista
Monthly notices of the Royal Astronomical Society
Data de publicació
2013-05
Volum
431
Número
3
Pàgina inicial
2778
Pàgina final
2788
DOI
https://doi.org/10.1093/mnras/stt374 Obrir en finestra nova
Resum
It has long been accepted that a possible mechanism for explaining the existence of magnetic white dwarfs is the merger of two white dwarfs, as there are viable mechanisms for producing sustainable magnetic fields within the merger product. However, the lack of rapid rotators in the magnetic white dwarf population has always been considered a problematic issue of this scenario. Smoothed particle hydrodynamics simulations show that in mergers in which the two white dwarfs have different masses, a...
Paraules clau
accretion, accretion discs, stars: magnetic field, white dwarfs
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

Participants

  • Kulebi, Baybar  (autor)
  • Eksi, K. Y.  (autor)
  • Loren Aguilar, Pablo  (autor)
  • Garcia-berro Montilla, Enrique  (autor)
  • Isern Vilaboy, Jordi  (autor)