Axisymmetric magnetic modes of neutron stars having mixed poloidal and toroidal magnetic fields
Author:
Affiliation:
1. Astronomical Institute, Tohoku University, Sendai, Miyagi 980-8578, Japan
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/476/3/3399/24476364/sty406.pdf
Reference41 articles.
1. Stability of magnetic fields in non-barotropic stars: an analytic treatment
2. AXISYMMETRIC TOROIDAL MODES OF GENERAL RELATIVISTIC MAGNETIZED NEUTRON STAR MODELS
3. Non-radial oscillations of the magnetized rotating stars with purely toroidal magnetic fields
4. Non-axisymmetric magnetic modes of neutron stars with purely poloidal magnetic fields
5. Alfvén QPOs in magnetars in the anelastic approximation
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1. Detecting deep axisymmetric toroidal magnetic fields in stars;Astronomy & Astrophysics;2022-05
2. Role of vector channel in different classes of (non) magnetized neutron stars;The European Physical Journal A;2020-04
3. Effects of a strong magnetic field on internal gravity waves: trapping, phase mixing, reflection, and dynamical chaos;Monthly Notices of the Royal Astronomical Society;2018-04-12
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