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 9.

Fourier transform of h × and h + for B p = B 1.5 (lower magenta line), B 3.5 (intermediate blue line), and B 6.5 (upper black line), assuming a source distance of 10 kpc. The vertical line marks a frequency of 1850 Hz.

Other Images in This Article
Copyright and Terms & Conditions