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The Energy Dependence of Neutron Star Surface Modes and X‐Ray Burst Oscillations

  • Authors: Anthony L. Piro and Lars Bildsten

Piro & Bildsten 2006 The Astrophysical Journal 638 968.

  • Provider: AAS Journals

Caption: Fig. 2.

Same as Fig. 1, but with ﹩\nu =600﹩ Hz and ﹩i=90^{\circ }﹩, and varying q and R for the numerical calculations. Setting ﹩R=20﹩ km (long dashed line) has the effect of decreasing the amplitude at high energies; compare this to the solid line. Decreasing q from 200 to 10 (dotted line) affects the energy dependence very little, showing that it is difficult to constrain the surface pattern created by the mode.

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