Topic033: Universal Aging V, Vertical Sequences II, Bill Tifft, 1/05/17
Book figures Appendix 1, figures 9 and 10
Book figure Appendix 1, figure 5
This topic uses correlations of the breadth (dispersion) of spectral lines with properties of E galaxies to examine effects of reinforcing (R) or opposed (O) offsets due to orientation of the nuclear quantum dipole. The previous topic examined the effects on rotation measures. Observed dispersions includes normal velocity dispersion, bulk motion effects of expansion and rotation variation along the line of sight, and the intrinsic dipole orientation effect. Dispersion in early type galaxies is rarely less than 100 km/s and closely related to their luminosity. Using absolute magnitudes derived from the standard Hubble flow (with some local classical dynamical distortions which I will note later) differential distances of sources is of no concern. The galaxy eccentricity (symbol Greek epsilon) is closely equivalent to morphology, even within…
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