Rotating neutron star models with a toroidal magnetic field - SFB/TR7
Rotating neutron star models with a toroidal magnetic field - SFB/TR7
Rotating neutron star models with a toroidal magnetic field - SFB/TR7
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Results for an n=1 polytropic equation of state<br />
10<br />
1<br />
0.9<br />
0.8<br />
(Bp/5.34 × 10 17 G) 2<br />
0.7<br />
0.6<br />
0.5<br />
0.4<br />
0.3<br />
1<br />
0.95<br />
0.85<br />
0.75 0.7<br />
Isocontours of ratio r p /r e of polar<br />
to equatorial radius as a function<br />
of peak <strong>magnetic</strong> <strong>field</strong> strength<br />
and rotation frequency for an M =<br />
1.4 M ⊙ model <strong>with</strong> a circumferential<br />
radius of R = 12km in the nonmagnetized<br />
case.<br />
0.2<br />
0.65<br />
0.1<br />
0.9<br />
0.8<br />
0.6<br />
0<br />
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1<br />
( f /828 Hz) 2<br />
Joachim Frieben Golm, June 18, 2007