The distribution of galaxy pair redshifts |
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| Authors: | T E Nordgren Y Terzian E E Salpeter |
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| Institution: | (1) Cornell University, 14853 Ithaca, New York |
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| Abstract: | High signal to noise neutral hydrogen observations of a complete sample of 132 galaxy pairs show a velocity difference distribution which decreases monotonically from zero. There is no strong indication of redshift periodicity for the entire sample and no indication at all for a subset of 79isolated galaxy pairs. In addition, when redshifts are corrected for the solar motion around the Galactic Center there is no indication of a redshift periodicity of 37.6 km s–1 in  V for galaxy pairs (as suggested by Guthrie and Napier 1996). |
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