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On the possible observational signatures of white dwarf dynamical interactions

Autor
Aznar, G.; Garcia-berro, E.; Magnien, M.; Loren, P.
Tipus d'activitat
Article en revista
Revista
Monthly notices of the Royal Astronomical Society
Data de publicació
2014-09-21
Volum
443
Número
3
Pàgina inicial
2372
Pàgina final
2383
DOI
https://doi.org/10.1093/mnras/stu1309 Obrir en finestra nova
Resum
We compute the possible observational signatures of white dwarf dynamical interactions in dense stellar environments. Specifically, we compute the emission of gravitational waves, and we compare it with the sensitivity curves of planned space-borne gravitational wave detectors. We also compute the light curves for those interactions in which a detonation occurs, and one of the stars is destroyed, as well as the corresponding neutrino luminosities. We find that for the three possible outcomes of ...
Paraules clau
Binaries: Close, Gravitational Waves, Neutrinos, Radiation Mechanisms: General, Radiation Mechanisms: Non-thermal, Supernovae: General, White Dwarfs
Grup de recerca
CTE-CRAE - Grup de Recerca en Ciències i Tecnologies de l'Espai
GAA - Grup d'Astronomia i Astrofísica

Participants

  • Aznar Siguan, Gabriela  (autor)
  • Garcia-berro Montilla, Enrique  (autor)
  • Magnien, Marie  (autor)
  • Loren Aguilar, Pablo  (autor)