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Magnetic white dwarfs: Observations, theory and future prospects

Autor
Garcia-berro, E.; Kilic, M.; Kepler, S.
Tipus d'activitat
Article en revista
Revista
International journal of modern physics D
Data de publicació
2016-01
Volum
25
Número
1
DOI
https://doi.org/10.1142/S0218271816300056 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/104215 Obrir en finestra nova
URL
http://www.worldscientific.com/doi/abs/10.1142/S0218271816300056 Obrir en finestra nova
Resum
Isolated magnetic white dwarfs have field strengths ranging from 10(3)G to 10(9) G, and constitute an interesting class of objects. The origin of the magnetic field is still the subject of a hot debate. Whether these fields are fossil, hence the remnants of original weak magnetic fields amplified during the course of the evolution of the progenitor of white dwarfs, or on the contrary, are the result of binary interactions or, finally, other physical mechanisms that could produce such large magne...
Citació
Garcia-berro, E., Kilic, M., Kepler, S. Magnetic white dwarfs: Observations, theory and future prospects. "International journal of modern physics D", Gener 2016, vol. 25, núm. 1.
Paraules clau
Stars, magnetic fields, stars: white dwarfs
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

Participants

  • Garcia-berro Montilla, Enrique  (autor)
  • Kilic, Mukremin  (autor)
  • Kepler, S.O.  (autor)

Arxius