Image Details

Choose export citation format:

Poloidal-field Instability in Magnetized Relativistic Stars

  • Authors: Riccardo Ciolfi and Luciano Rezzolla

Ciolfi & Rezzolla 2012 The Astrophysical Journal 760 1.

  • Provider: AAS Journals

Caption: Figure 10.

h rss vs. B p in Gauss assuming a distance of 10 kpc and a damping time of τ GW = 100 ms. Horizontal lines mark the strain-noise amplitude of the considered GW detectors at the f-mode frequency f 0. Finally, the red line is obtained by imposing a quadratic scaling (∝ B 2) and fitting the results for the lowest magnetic fields (first four points).

Other Images in This Article
Copyright and Terms & Conditions