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Synchrotron Self‐Compton Model for PKS 2155−304

  • Authors: Masaaki Kusunose and Fumio Takahara

Kusunose & Takahara 2008 The Astrophysical Journal 682 784.

  • Provider: AAS Journals

Caption: Fig. 4.

Time evolution of SED of model A is shown. The SEDs are plotted at every ﹩R/ c﹩ and evolve from lower to upper lines. Labels are ﹩t/ ( R/ c) ﹩ in the comoving frame.

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