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1“... section of the Local Void, where the density of galaxies with radial velocities below 3000 km/s is rather...”
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2“... group around NGC3379 = Leo I and NGC3627 as well as the Local Group show the motion from the Local Void...”
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3“... (kSZ) effect. Our study is based on the large local void (LLV) radial profile observed by Keenan...”
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