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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 3.

(a) VLBA images at 8.4 (top left), 15.3 (top right), and 22.2 GHz (bottom) from epoch 1. In each case the bottom contour is 0.1 mJy/beam increasing in factors of 2. The data have been weighted with Briggs’ weighting scheme (Briggs 1995) using a robustness parameter of 0. (b) VLBA images at 8.4 (top left), 15.3 (top right), and 22.2 GHz (bottom) from epoch 2. In each case the bottom contour is 0.1 mJy/beam increasing in factors of 2. The data have been weighted with Briggs’ weighting scheme (Briggs 1995) using a robustness parameter of 0. (c) VLBA images at 8.4 (top left), 15.3 (top right), and 22.2 GHz (bottom) from epoch 3. In each case the bottom contour is 0.1 mJy/beam increasing in factors of 2. The data have been weighted with Briggs’ weighting scheme (Briggs 1995) using a robustness parameter of 0. (d) VLBA images at 8.4 (top left), 15.3 (top right), and 22.2 GHz (bottom) from epoch 4. In each case the bottom contour is 0.1 mJy/beam increasing in factors of 2. The data have been weighted with Briggs’ weighting scheme (Briggs 1995) using a robustness parameter of 0.

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