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The Relativistic Jet-accretion Flow–wind Connection in Mrk 231

  • Authors: Cormac Reynolds, Brian Punsly, Giovanni Miniutti, Christopher P. O'Dea, and Natasha Hurley-Walker

2017 The Astrophysical Journal 836 155.

  • Provider: AAS Journals

Caption: Figure 8.

Top frame shows the shift of the core as a function of frequency in epoch 4 due to SSA opacity effects. The fits of the power laws to the data are good as evidenced by the large squared multiple regression values, R2. The quantity, x, in the equation for the core shift is the observed frequency in GHz. The bottom frame shows the shifted true core location that is consistent with zero offset at high frequency in the top frame.

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