Abstract
WE have derived1 the solar motion with respect to galaxies at different distances and have shown how the solar apex varies systematically with the distance of the reference objects.
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References
Vaucouleurs, G. de, and Peters, W. L., Nature, 220, 868 (1968).
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Kerr, F. J., and Sullivan, W. T., Astrophys. J. (in the press).
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VAUCOULEURS, G., PETERS, W. Solar Motion with Respect to the High-velocity HI Clouds and to the Local Group. Nature 223, 938 (1969). https://doi.org/10.1038/223938a0
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DOI: https://doi.org/10.1038/223938a0
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