Galoot said:
Nereid said:
Except that the quasars seem to be just active galaxy nuclei with normal galaxies around them (the 'quasar host', as it's called) ... at distances from us consistent with their redshifts (i.e. vastly further away than the galaxy Arp claims they've been ejected from).
I'm not sure if I follow. As you say, quasars are always (as far I know) been found associated with a host galaxy. For the quasars in Alp's atlas, the only nearby (visually) galaxies which could serve as the host galaxies (and which likely are due to the observed dust bridges) are ones with dramatically different redshifts. How does that show Alp to be wrong? Alp and Burbrige even claimed just a year ago to have found a quasar with larger redshift embedded in, or possibly immediately in front of, the galaxy NGC 7319. How could a quasar so far away (if it is far away) be seen clearly through the dust of the central core of a galaxy?
The confusion here is 'host'; the host galaxies of quasars (those that have been reliably observed, to date) are very, very close (on the sky) to the photocentre of the quasar ... mostly <2" ... and they surround the photocentre on all sides.
The 'host galaxies' that you seem to be referring to are those which Arp (and followers) identify as the 'parent' from which the quasar was ejected ... they are almost always >10" away from the nucleus (and in some cases 30' or more), and in only a few cases are the purported 'child' quasars within the 'sky isophotes' of the 'parent'.
Another curious thing (if you're an Arpian): the sizes and colours of those host galaxies (the real ones, not the Arpian fictions) which have been reliably detected are quite consistent with those of galaxies at the distance that the redshift of the quasar implies (via the Hubble relationship).
NGC 7319 is an excellent example of the sloppy statistics I referred to above - given the observed sky density of quasars, that of large (on the sky) galaxies, and the well-observed gravitational lensing of background objects that appear near galaxies, an object like the 'quasar within NGC 7319' is entirely unexceptional.
It's not difficult to find curious alignments - one of my favourites is
CG4. The hard part is doing the statistics to show when something curious is more than a chance alignment. As I said earlier, the Arpians have a miserable track record in this regard.
That assumes what is the scope and nature of the cause of the quasar redshift. Quasars are thought to be rather small, on the order of a singularity up to about the size of our solar system, from what I've read. If the cause of the redshift is a halo of diffuse plasma around the quasar, as postulated by Brynjolfsson, then the light emitting from the compact quasar could be shifted without affecting the light from dust bridges many hundreds or thousands of light years away.
Indeed. However that would take us beyond the scope of this section of PF - Brynjolfsson's ideas are very clearly non-mainstream (and, I suspect, strongly inconsistent with many many more very good observational and experimental results than Arp's are).