ar X iv : a st ro - p h / 03 06 04 2 v 1 2 J un 2 00 3 Intrinsic Redshifts in QSOs Near NGC 6212

ar X iv : a st ro - p h / 01 12 04 5 v 1 3 D ec 2 00 1 On QSO Distances and Lifetimes in a Local Model

It was shown previously from the redshifts and positions of the compact, high-redshift objects near the Seyfert galaxy NGC 1068 that they appear to have been ejected from the center of the galaxy in four similarly structured triplets. In this local scenario, they lie at the distance of NGC 1068, a distance much closer than a cosmological interpretation of their redshifts would imply. A large po...

ar X iv : a st ro - p h / 03 05 06 0 v 1 5 M ay 2 00 3 Intrinsic Redshifts and the Hubble Constant

We show that the V CMB velocities of the Fundamental Plane (FP) clusters studied in the Hubble Key Project appear to contain the same discrete " velocities " found previously by us and by Tifft to be present in normal galaxies. Although there is a particular Hubble constant associated with our findings we make no claim that its accuracy is better than that found by the Hubble Key Project. We do...

ar X iv : a st ro - p h / 01 11 12 3 v 1 6 N ov 2 00 1 Further Evidence for Large Intrinsic Redshifts

An examination of the positions and redshifts of the compact, QSO-like objects reported near the Seyfert 2 galaxy NGC 1068 has revealed many relationships that suggest strongly that the objects have been ejected from the galaxy. Although some of the same relations have been found for the compact objects near NGC 3516, the higher number of sources near NGC 1068 has resulted in a detailed physica...

ar X iv : a st ro - p h / 02 04 03 6 v 1 2 A pr 2 00 2 Investigating the Flame Microstructure in Type

ar X iv : a st ro - p h / 06 04 34 7 v 1 1 7 A pr 2 00 6 Spitzer Observations of High Redshift QSOs

We have observed 13 z ≥ 4.5 QSOs using the Multiband Imaging Photometer for Spitzer, nine of which were also observed with the Infrared Array Camera. The observations probe rest wavelengths ∼ 0.6 − 4.3µm, bracketing the local minimum in QSO spectral energy distributions (SEDs) between strong optical emission associated directly with accretion processes and thermal emission from hot dust heated ...