89 citations · 228 across the 7 of their papers we have counts for
7 papers
Magnetic winding and turbulence in ultra-hot Jupiters
Clàudia Soriano-Guerrero, Daniele Viganò, Rosalba Perna +2
While magnetism in exoplanets remains largely unknown, Hot Jupiters have been considered as natural candidates to harbour intense magnetic fields, both due to their large masses an…
The force-free twisted magnetosphere of a neutron star - II: Degeneracies of the Grad-Shafranov equation
Taner Akgün, Pablo Cerdá-Durán, Juan Antonio Miralles +1
We extend our previous study of equilibrium solutions of non-rotating force-free magnetospheres of neutron stars. We show that multiple solutions exist for the same sets of paramet…
Long-term evolution of the force-free twisted magnetosphere of a magnetar
Taner Akgün, Pablo Cerdá-Durán, Juan Antonio Miralles +1
We study the long-term quasi-steady evolution of the force-free magnetosphere of a magnetar coupled to its internal magnetic field. We find that magnetospheric currents can be main…
The relevance of ambipolar diffusion for neutron star evolution
Andrea Passamonti, Taner Akgün, José A. Pons +1
We study ambipolar diffusion in strongly magnetised neutron stars, with special focus on the effects of neutrino reaction rates and the impact of a superfluid/superconducting trans…
The force-free twisted magnetosphere of a neutron star
Taner Akgün, Juan Antonio Miralles, José A. Pons +1
We present a detailed analysis of the properties of twisted, force-free magnetospheres of non-rotating neutron stars, which are of interest in the modelling of magnetar properties…
CP and related phenomena in the context of Stellar Evolution
J. Braithwaite, T. Akgün, E. Alecian +13
We review the interaction in intermediate and high mass stars between their evolution and magnetic and chemical properties. We describe the theory of Ap-star `fossil' fields, befor…
Precession of the Isolated Neutron Star PSR B1828-11
Taner Akgun, Bennett Link, Ira Wasserman
Stairs, Lyne & Shemar have found that arrival time residuals from PSR B1828-11 vary periodically with a period of 500 days. This behavior can be accounted for by precession of the…