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Rossby numbers of fully convective and partially convective stars
(Proceedings of the International Astronomical Union, 2019)
Stability of hall equilibria in neutron star crusts
(Institute of Physics Publishing, 2014)
© 2014. The American Astronomical Society. All rights reserved.. In the solid crusts of neutron stars, the advection of the magnetic field by the current-carrying electrons, an effect known as Hall drift, should play a ...
Binarity Versus Magnetic Fields in Upper Main-sequence Stars
(University of Zagreb, 2013-01)
We review the status of the work on the detection, possible origin, and modelling of magnetic fields in binary systems with intermediate- and higher-mass primaries at different evolutionary stages. This review also includes ...
Evolution of magnetic field and spin period in accreting neutron stars
(Edp Sciences S A, 2014)
Magnetic fields of HgMn stars
(EDP Sciences, 2012-11)
Context. The frequent presence of weak magnetic fields on the surface of spotted late-B stars with HgMn peculiarity in binary systems has been controversial during the two last decades. Recent studies of magnetic fields ...
Instability of magnetic equilibria in barotropic stars
(Oxford University Press, 2015)
In stably stratified stars, numerical magnetohydrodynamics simulations have shown that arbitrary
initial magnetic fields evolve into stable equilibrium configurations, usually containing
nearly axisymmetric, linked ...
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars
(EDP Sciences, 2013-03)
Context. Theories on the origin of magnetic fields in massive stars
remain poorly developed, because the properties of their magnetic field
as function of stellar parameters could not yet be investigated.
Additional ...
On magnetic equilibria in barotropic stars
(IOP PUBLISHING, 2015)
Upper main-sequence stars, white dwarfs, and neutron stars are known to possess stable, large-scale magnetic fields. Numerical works have confirmed that stable magnetohydrodynamic equilibria can exist in non-barotropic, ...