Then why bother with his theory? If it cannot give the distance of "certain types of objects" then what use is it?
So now the litmus test of a cosmological theory is whether it tells one the distance to objects? Saying "I don't know" is to not allowed in mainstream thinking? Maybe that's why they find it necessary to invent gnome after gnome. Because they don't feel comfortable just saying "I don't know".
As I said there are various theories to explain these observations.
Again, you haven't offered any theories to explain them. You haven't linked us to any peer reviewed papers explaining them. You haven't quoted any published article in scientific magazines. You are just waving your hands hoping the observations they will go away.
Originally Posted by BeAChooser
The very notion of an expanding universe came about because redshifts seem to suggest one ... one where everything must have had an initial origin back in time. ... snip ...
Have you ever heard of Hubble and his constant? The experimental results started with his paper in 1929 after he worked for a decade when a steady state universe was accepted. He fit a straight line to the data without Big Bang cosmology.
That's not a correct rendition of history, RC. Vesto Slipher started measuring the Doppler shift of galaxies about 1910, although at the time he didn't know that's what they were ... he called them nebula. Almost all of the objects showed a redshift which suggested the objects were collectively moving away from us. That is where matters stood until 1922 when Friedmann derived equations from Einstein's theory of General Relativity that suggested the universe should either be expanding or collapsing. In 1924, Hubble measured the distance to the nearest spiral "nebula" and showed that they weren't nebula at all, but other galaxies filled with stars just like the Milky Way. In 1927, Georges Lemaître independently derived Friedmann's equations and for the first time, it was concluded in a paper that the recession of the objects was due to the expansion "of the universe". His model included a redshift/distance relationship similar to that which in 1929 Hubble and Humason obtained by fitting a line through the observational data that had been collected so far. However, it wasn't until 1931 that Lemaître actually published a paper suggesting that the universe began as a simple "primeval atom" or "cosmic egg". Therefore, one might consider 1931 as the real birthdate of the *Big Bang* theory, in which case, redshifts are "one of the foundations of the Big Bang cosmology". Like I said. And if the redshift/distance formula doesn't actually hold for many objects ...
The paper has z intervals of 0.258, 0.312, 0.44, 0.63, and 1.1 so:
• Paper: z = 0.258, 0.57, 1.01, 1.64, 2.74
• You: z = 0.061, 0.30, 0.60, 0.91, 1.41, 1.96
To my mind that is really different.
Actually, the paper does mention the sequence might start at z=0.062. So let's line them up again with that in mind.
Harnett's Paper:
z = 0.06, 0.26, 0.57, 1.01, 1.64, 2.74
Burbidge and Napier (2000) /Karlsson/Arp:
z = 0.06, 0.30, 0.60, 0.91, 1.41, 1.96
Sorry but that doesn't look all that different considering all the possible factors that might cause a difference. You know that there are uncertainties in any given calculation of this sort, especially as you go farther out.
How about we add some further data by another author:
http://arxiv.org/pdf/astro-ph/0411548 "Intrinsically faint quasars: evidence for meV axion dark matter in the Universe, Anatoly A. Svidzinsky, November 18, 2004 ... snip ... Growing amount of observations indicate presence of intrinsically faint quasar subgroup (a few % of known quasars) with noncosmological quantized redshift. Here we find an analytical solution of Einstein equations describing bubbles made from axions with periodic interaction potential. Such particles are currently considered as one of the leading dark matter candidate. The bubble interior possesses equal gravitational redshift which can have any value between zero and infinity. Quantum pressure supports the bubble against collapse and yields states stable on the scale more then hundreds million years. Our results explain the observed quantization of quasar redshift and suggest that intrinsically faint point-like quasars associated with nearby galaxies are axionic bubbles ... snip ... . They are born in active galaxies and ejected into surrounding space. Properties of such quasars unambiguously indicate presence of axion dark matter in the Universe and yield the axion mass m ? 1 meV, which fits in the open axion mass window constrained by astrophysical and cosmological arguments." This source lists quantization at:
z = X.XX, 0.36, 0.63, 0.96, 1.40, 2.06
That again seems to line up relatively well.
Also, are you aware (
http://www.eitgaastra.nl/timesgr/part5/4.html ) that "there is a difference between radio quasars redshifts in the Right Ascension = 0 hour region (peaks at .30, .60, .96, 1.41, 1.96) relative to the Right Ascension = 12 hour region (peaks at .34, .65, 1.02, 1.48, 2.05)29." That might explain some of the variation too.
What a coincidence that the redshifts in all the examples of curious alignments I listed or quasars in front of low redshift galaxies or the bullet cluster case just happen to have redshifts near one of these peaks. Just a coincidence. Right?
These five overdense regions lying in a narrow redshift range indicate the presence of a supercluster in this field
That speculation is perhaps another gnome. Do you have any confirmation that all 5 objects are part of a supercluster? How many foreground and background objects are there in the field? And do all the supercluster members have a redshift within 0.01 of the others?
Overall, we show that the properties of this supercluster are similar to the well-studied Shapley and Hercules superclusters at lower redshift
Well let's look at the spread of redshifts in the Shapely supercluster which has somewhat over 700 members. Here's a source (
http://arxiv.org/pdf/astro-ph/9903028 ) with histograms of redshifts for the Shapely cluster and in the direction of that supercluster. Note that three quarters of them have velocities in the range 7580 to 18300 kms (where 18300 km/s corresponds to z of about 0.061) and the rest are outside that range. So that means that three quarters of the members have z ranging from 0.025 to 0.061. So what are the odds that if you picked 5 of them at random you'd end up with all 5 being within 0.01? Pretty slim? That source also notes that there is a foreground wall of 269 galaxies with quite different redshifts (z = 0.067 to 0.02). What are the odds that one of them wouldn't be picked randomly in a sample of 5? I think you are hand waving, RC.
And you might find this interesting:
http://www.springerlink.com/content/qt7454133824p423/ "On the investigations of galaxy redshift periodicity, K.*Bajan, P.*Flin, W.*Godlowski, and V.*N.*Pervushin, 2006, ... snip ... We conclude that galaxy redshift periodization is an effect which can really exist." That reference has a histogram of radial velocities for the Hercules cluster. Again, we see that z has a very large range ... far more than 0.01.
Remember that 30 Mpc is smaller than the Local Group.]
Let's look at redshifts in the Local Group. It consists of about 30 galaxies. The Andromeda galaxy is one of them. And guess what? It's moving towards us at about 50 km/s. Wonder what the rest are doing?
