Fig. 1 from A Large‐scale Bulk Flow of Galaxy Clusters

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A Large‐scale Bulk Flow of Galaxy Clusters

Authors: Michael J. Hudson, Russell J. Smith, John R. Lucey, David J. Schlegel, and Roger L. Davies

Hudson et al. 1999 The Astrophysical Journal Letters 512 L79.

Provider: AAS Journals

Caption: Fig. 1.

Peculiar velocities as a function of angle from the apex of the bulk flow. Symbol sizes are inversely proportional to errors. The solid line is the best‐fitting bulk flow model, and clusters that deviate from this flow at the 2 σ level are indicated, with error bars.

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