Abstract
If the standard interpretation of the dipole anisotropy in the microwave background radiation as being due to our peculiar velocity in a homogeneous isotropic universe is correct, then radio-source number counts must show a similar anisotropy. Conversely, determination of a dipole anisotropy in those counts determines our velocity relative to their rest frame; this velocity must agree with that determined from the microwave background radiation anisotropy. Present limits show reasonable agreement between these velocities.
Cite
CITATION STYLE
Ellis, G. F. R., & Baldwin, J. E. (1984). On the expected anisotropy of radio source counts. Monthly Notices of the Royal Astronomical Society, 206(2), 377–381. https://doi.org/10.1093/mnras/206.2.377
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