17.07.2013 Views

Observational Evidence Favors a Static Universe - Journal of ...

Observational Evidence Favors a Static Universe - Journal of ...

Observational Evidence Favors a Static Universe - Journal of ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

unity. Note that the critical difference from BB is in the size <strong>of</strong> the radii. They<br />

are not only much closer to the nearby galaxy radii but because they are larger<br />

they do not require the non-linear corrections for the Kormendy relation. As<br />

before we note that the nearby galaxies are BCG which may have a brighter<br />

SB than the normal field galaxies. If this is true it would bias the exponent<br />

to a larger value. If we assume that CC is correct then this data shows that<br />

on average the BCG galaxies are −0.64 ± 0.08 mag (which is a factor <strong>of</strong> 1.8 in<br />

luminosity) brighter than the general cluster galaxies.<br />

4.1.3 Conclusion for surface brightness<br />

The SL01 data for the surface brightness <strong>of</strong> elliptic galaxies is consistent with<br />

BB but only if a large unknown effect <strong>of</strong> luminosity evolution is included. The<br />

data do not support expansion and are in complete agreement with CC.<br />

4.2 Angular size<br />

Closely related to surface brightness is relationship between the observed angu-<br />

lar size <strong>of</strong> a distant object and its actual linear transverse size. The variation<br />

<strong>of</strong> angular size as a function <strong>of</strong> redshift is one <strong>of</strong> the tests that should clearly<br />

distinguish between BB and CC. The major distinction is that CC like all tired-<br />

light cosmologies does not include the (1 + z) aberration factor. Its relationship<br />

(Eq. 12) between the observed angular size and the linear size is very close (for<br />

small redshifts) to the Euclidean equation. Gurvits, Kellermann & Frey (1999)<br />

provide a comprehensive history <strong>of</strong> studies for a wide range <strong>of</strong> objects that gen-<br />

erally show a 1/z or Euclidean dependence. Most observers suggest that the<br />

probable cause is some form <strong>of</strong> size evolution. Recently Lopez-Corredoira (2010)<br />

23

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!