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Cited article:
L. Bonanno , C. Cuofano , A. Drago , G. Pagliara , J. Schaffner-Bielich
A&A, 532 (2011) A15
Published online: 2011-07-13
This article has been cited by the following article(s):
5 articles
The role of magnetic damping in the r-mode evolution of accreting neutron stars
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Growth of magnetic fields in accreting millisecond pulsars
C. Cuofano, A. Drago and G. Pagliara Monthly Notices of the Royal Astronomical Society 428 (2) 1438 (2013) https://doi.org/10.1093/mnras/sts134
Nuclear symmetry energy and ther-mode instability of neutron stars
Isaac Vidaña Physical Review C 85 (4) (2012) https://doi.org/10.1103/PhysRevC.85.045808
An r-mode in a magnetic rotating spherical layer: application to neutron stars
S. Abbassi, M. Rieutord and V. Rezania Monthly Notices of the Royal Astronomical Society 419 (4) 2893 (2012) https://doi.org/10.1111/j.1365-2966.2011.19930.x
Generation of strong magnetic fields byr-modes in millisecond accreting neutron stars: Induced deformations and gravitational wave emission
Carmine Cuofano, Simone Dall’Osso, Alessandro Drago and Luigi Stella Physical Review D 86 (4) (2012) https://doi.org/10.1103/PhysRevD.86.044004