Abstract
The variation of radio luminosity with redshift and its effect on the analysis of the angular size-redshift (θ –z) relation for a bright radio source sample (s 178 ≥ 10Jy) has been investigated. By assuming a power law dependence of luminosity on redshift of the formP ∼ (1 +z)β, it was found thatβ ≈ 4.4 (with correlation coefficientr ≈ 0.99) for at leastz ≥ 0.3. Correction for such a strongP – (1 +z) correlation when considering theθ –z data for the sample led to a steeperθ –z slope. This could be explained by assuming linear size evolution of the formD ∼ (1 +z)−n withn = 2.8 – 3.3 consistent with both theoretical results and those obtained for more homogeneous source samples.
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Ubachukwu, A.A. The effect of luminosity-redshift correlation on the analysis of the angular size-redshift relation for radio galaxies. Astrophys Space Sci 232, 23–25 (1995). https://doi.org/10.1007/BF00627540
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DOI: https://doi.org/10.1007/BF00627540