A cyclotron absorption line as used in pulsar spectra. See Mihara et al., Nature, 1990 or Makishima et al. PASJ, 1990.
![M(E) = exp[-D_f*(W_f*E/E_cycl)^2/((E-E_cycl)^2+W_f^2) + D_2h*(W_2h*E/(2E_cycl))^2/((E-2E_cycl)^2+W_2h^2)]](XSmodelCyclabs_files/image001.gif)
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par1= Df |
depth of the fundamental |
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par2= Ecycl |
cyclotron energy |
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par3= Wf |
width of the fundamental |
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par4= D2h |
depth 2nd harmonic |
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par5= W2h |
width of the 2nd harmonic |