Flattening modulus of a neutron star by rotation and magnetic field

Details Flattening modulus of a neutron star by rotation and magnetic field Flattening modulus of a neutron star by rotation and magnetic field

2000-01-22

arxiv.org/abs/astro-ph/0001397v1

Astron.Astrophys.356:234-237,2000

Astronomy and Astrophysics

Astrophysics

5 pages, 4 figures, accepted for publication in Astronomy and Astrophysics

Scientific paper

We calculated the ellipticity of the deformed star due to the rotation or
magnetic field. These two effects are compared to each other within general
relativity. It turned out that the magnetic distortion is important for
recently observed candidates of magnetars, while the magnetic effect can be
neglected for well-known typical pulsars.

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