pogo wrote:You are not reading WP correctly, no. None of those are quasars.
An optically violent variable quasar (often abbreviated as OVV quasar) is a type of highly variable quasar. It is a subtype of blazar that consists of a few rare, bright radio galaxies, whose visible light output can change by 50% in a day.[2]
They are similar in appearance to BL Lacs but generally have a stronger broad emission line, and tend to have higher red shift components.
https://en.wikipedia.org/wiki/OVV_quasar
You might be right about that, but that article is very short, no mention of polarisation either way.
This is more like it:
Blazars, like all AGN, are thought to be ultimately powered by material falling onto a supermassive black hole at the center of the host galaxy. Gas, dust and the occasional star are captured and spiral into this central black hole creating a hot accretion disk which generates enormous amounts of energy in the form of photons, electrons, positrons and other elementary particles. This region is quite small, approximately 10−3 parsecs in size.
There is also a larger opaque toroid extending several parsecs from the central black hole, containing a hot gas with embedded regions of higher density. These "clouds" can absorb and then re-emit energy from regions closer to the black hole. On Earth the clouds are detected as emission lines in the blazar spectrum.
Perpendicular to the accretion disk, a pair of relativistic jets carries a highly energetic plasma away from the AGN. The jet is collimated by a combination of intense magnetic fields and powerful winds from the accretion disk and toroid. Inside the jet, high energy photons and particles interact with each other and the strong magnetic field. These relativistic jets can extend as far as many tens of kiloparsecs from the central black hole.
All of these regions can produce a variety of observed energy, mostly in the form of a nonthermal spectrum ranging from very low frequency radio to extremely energetic gamma rays, with a high polarization (typically a few percent) at some frequencies.
https://en.wikipedia.org/wiki/Blazar
But your most glaring mistakes are in basic science, which is what relativity is.
Science is experiments, not dogma.
... everything – matter and light in particular – are all affected by gravity the same way. If it wasn’t, over the vast distances of space, it would be very very obvious.
This is a singular phenomenon, that occurs rarely in exceptional circumstances. Someone might have looked at it, but they equally might not have. You'd have to be looking at the polarisation of light after gravitational lensing to have any chance of spotting it experimentally.
pogo wrote:It’s particularly pertinent here as gravitational lensing is one of the key predictions of general relativity. Predicted by Einstein in the 1930s but not observed for another 40 years. It’s only one of the many bits of evidence we have for general relativity.
History
Henry Cavendish in 1784 (in an unpublished manuscript) and Johann Georg von Soldner in 1801 (published in 1804) had pointed out that Newtonian gravity predicts that starlight will bend around a massive object.[6] The same value as Soldner's was calculated by Einstein in 1911 based on the equivalence principle alone. However, Einstein noted in 1915 in the process of completing general relativity, that his (and thus Soldner's) 1911-result is only half of the correct value. Einstein became the first to calculate the correct value for light bending.[7]
https://en.wikipedia.org/wiki/Gravitational_lens
"My way is the way of not fighting":- the book of Enter the Dragon.