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Rotating neutron star models with a toroidal magnetic field - SFB/TR7

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12<br />

Results for an n=1 polytropic equation of state<br />

10 −2<br />

10 −3<br />

10 −4<br />

10 −5<br />

Bonazzola & Gourgoulhon (1996)<br />

Cutler (2002)<br />

Magnetic distortion ɛ B as a<br />

function of circumferential<br />

radius R at fixed average<br />

<strong>magnetic</strong> <strong>field</strong> strength for<br />

a non-rotating M = 1.4 M ⊙<br />

model computed according<br />

to Bonazzola & Gourgoulhon<br />

(1996) and Cutler<br />

(2002) respectively.<br />

−ǫ B<br />

10 1 10 2<br />

10 −6<br />

R [km]<br />

Joachim Frieben Golm, June 18, 2007

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