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Tully–Fisher Distances for Southern Galaxies with HIPASS and WISE

  • Authors: J. R. Sheil, M. J. I. Brown, and V. Parkash

2020 Research Notes of the AAS 4 49.

  • Provider: AAS Journals

Caption: Figure 1.

The distribution of galaxies in the Southern sky (left) and recessional velocity as a function of Tully–Fisher distance (right). In the right panel the Hubble constant relation with 73.3 ± 1 km s−1 Mpc−1 is shown (red line) and the scatter of the distances about this relation indicates the 1σ uncertainties of our distances is 19.5%.

(The data used to create this figure are available.)

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