Let’s get ourselves up to speed on quasars. Not pointing fingers, but some of what I’m reading here makes me wonder if some of us aren’t working from a VERY old understanding of what quasars are.
They were first discovered in 1963, as point-sources of light that were not stars. Hence the name “quasi-stellar objects” or “quasars”.
The reason we know they are not stars is that stars have a radiation spectrum that falls into a certain pattern, but quasars did not. We also realized that they are fairly large and extremely far away.
In the mid-1990s, astronomers began to realize what they might be.
If you’ve ever seen an amazing photo of a galaxy and then looked at one live through a telescope, you notice a certain brilliance missing. That’s because to get the photo, it must be overexposed. Dim things achieve a more visible brightness, and bright things wash out to a very bright white.
Here is a fairly wide-field picture of Galaxy M33. It appears completely blown out.
In a tighter shot of M33. The overexposure has let us see some of the outer structure of the galaxy, but notice that the core is still washed out.
Here is an even tighter shot of the core area of M33. We can see more detail, but there is still a very bright area in the center that the overexposure has washed out.
So the closer we look at a galaxy, more we realize that there is a very bright point-source in the middle. Sound familiar?
What then, would be most visible about this galaxy if we were to observe it from 10-12 billion light-years away?
IOW, quasars are galaxy cores (specifically the cores of supermassive galaxies), which we’ve know for about 10 years.
More information here
The fact that they are so far away means that quasars represent an early stage of formation of such galaxies.