The proto-neutron-star dynamo. Viability and impediments
A&A, 435 1 (2005) 201-206
Published online: 2005-04-25
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
Neutrino-driven massive stellar explosions in 3D fostered by magnetic fields via turbulent α-effect
Jin Matsumoto, Tomoya Takiwaki and Kei KotakeMonthly Notices of the Royal Astronomical Society: Letters 528 (1) L96 (2023)
https://doi.org/10.1093/mnrasl/slad173
Convection and Dynamo in Newly Born Neutron Stars
Youhei Masada, Tomoya Takiwaki and Kei KotakeThe Astrophysical Journal 924 (2) 75 (2022)
https://doi.org/10.3847/1538-4357/ac34f6
Axisymmetric equilibrium models for magnetised neutron stars in scalar-tensor theories
J. Soldateschi, N. Bucciantini and L. Del ZannaAstronomy & Astrophysics 640 A44 (2020)
https://doi.org/10.1051/0004-6361/202037918
The convective instability of a Maxwell–Cattaneo fluid in the presence of a vertical magnetic field
I. A. Eltayeb, D. W. Hughes and M. R. E. ProctorProceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences 476 (2241) (2020)
https://doi.org/10.1098/rspa.2020.0494
Rotating stars in relativity
Vasileios Paschalidis and Nikolaos StergioulasLiving Reviews in Relativity 20 (1) (2017)
https://doi.org/10.1007/s41114-017-0008-x
General relativistic models for rotating magnetized neutron stars in conformally flat space–time
A. G. Pili, N. Bucciantini and L. Del ZannaMonthly Notices of the Royal Astronomical Society 470 (2) 2469 (2017)
https://doi.org/10.1093/mnras/stx1176
Influence of small-scale magnetic field on the reverse positron current in the inner gaps of radio pulsars
D. P. Barsukov, O. A. Goglichidze and A. I. TsyganAstronomy Reports 60 (6) 586 (2016)
https://doi.org/10.1134/S106377291604003X
The role of currents distribution in general relativistic equilibria of magnetized neutron stars
N. Bucciantini, A. G. Pili and L. Del ZannaMonthly Notices of the Royal Astronomical Society 447 (4) 3278 (2015)
https://doi.org/10.1093/mnras/stu2689
General relativistic neutron stars with twisted magnetosphere
A. G. Pili, N. Bucciantini and L. Del ZannaMonthly Notices of the Royal Astronomical Society 447 (3) 2821 (2015)
https://doi.org/10.1093/mnras/stu2628
Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition
A. G. Pili, N. Bucciantini and L. Del ZannaMonthly Notices of the Royal Astronomical Society 439 (4) 3541 (2014)
https://doi.org/10.1093/mnras/stu215
Neutron Stars and Pulsars
Ulrich GeppertAstrophysics and Space Science Library, Neutron Stars and Pulsars 357 319 (2009)
https://doi.org/10.1007/978-3-540-76965-1_13
Protoneutron star dynamos: pulsars, magnetars, and radio-silent X-ray emitting neutron stars
A. Bonanno, V. Urpin and G. BelvedereAstronomy & Astrophysics 451 (3) 1049 (2006)
https://doi.org/10.1051/0004-6361:20054473
Magnetars versus radio pulsars
U. Geppert and M. RheinhardtAstronomy & Astrophysics 456 (2) 639 (2006)
https://doi.org/10.1051/0004-6361:20065144
Dynamical Evolution of Neutrino‐cooled Accretion Disks: Detailed Microphysics, Lepton‐driven Convection, and Global Energetics
William H. Lee, Enrico Ramirez‐Ruiz and Dany PageThe Astrophysical Journal 632 (1) 421 (2005)
https://doi.org/10.1086/432373