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Seeking the Local Convergence Depth. IV. Tully‐Fisher Observations of 35 Abell Clusters

  • Authors: Daniel A. Dale, Riccardo Giovanelli, Martha P. Haynes, Eduardo Hardy, and Luis E. Campusano

Dale et al. 1999 The Astronomical Journal 118 1468.

  • Provider: AAS Journals

Caption: Fig. 2.

Sky and velocity distribution of galaxies in the clusters A2877, A2877b, and A160. Circles represent cluster members with measured photometry and widths; if unfilled, widths are poorly determined. For A2877b, triangles identify cluster members. Asterisks identify foreground and background galaxies, and dots show the location of galaxies with known redshift but lacking accurate width and/or photometry. Squares indicate outlines of imaged fields with the 0.9 m telescopes. Vertical dashed lines in the lower panels indicate 1RA (and 2RA for A160); a dotted line is used for A2877b. The top panels contain circles of radius 1RA (and 2RA for A160).

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