bapowell said:
Sure, except for those currently outside the cosmological event horizon. Recall that the particle horizon is currently inside the event horizon, so there are galaxies -- those that are in between the two horizons -- that are not currently observable but one day will be.
Brian, you're the professional so I'm worried that I may be using the words "cosmological event horizon" wrong. I hope you can help me get this sorted out.
I think the distance today to the CEH is about 16 billion LY. We may be observing a galaxy that is beyond that but if we send a message to them TODAY it will never get there. They are out of causal reach. If they do something today it will never affect us, if they have a supernova we will never see it.
I think that the
particle horizon distance as of today is about 46 billion LY. The matter we are currently getting CMB radiation from is now about 45 or 45.5 or something, but the actual particle horizon is a bit farther because we could, in principle have received light from slightly more distant stuff except for the opacity/glare. Or received neutrinos...etc.
I think in terms of today's distance (treated as a non-expanding label on matter, a so-called "comoving distance" label that doesn't change as the U expands) that there is a
limit to the particle horizon which is as I recall something like 63 billion LY.
If some matter is, today, farther than 63 billion LY then we will never get light from it, even light that it emitted way back in the past. That LIGHT is today still outside the 16 billion LY CEH range. So it can never reach us.
The figures are just approximate. I'm using numbers for concreteness sake. Dragon eyes might want to look up "proper distance" and "comoving distance" and maybe "cosmological event horizon". I don't know if wikipedia has an entry on all or some of those.
It seems to me (and I could be wrong) that I've always heard the term CEH used to refer to that 16 billion LY distance and never to refer to the 63 billion LY comoving distance which is the limit towards which the particle horizon (currently 46 or so) is tending. Some of this stuff is in the bottom panel of Lineweaver's Figure 1 here
http://ned.ipac.caltech.edu/level5/March03/Lineweaver/Figures/figure1.jpg
You can see that what he calls "event horizon" is about 16
and the ultimate limit (time = "infinity") of what he calls "particle horizon" is about 63.
Of course in the long run though we will still be receiving light from all those (then dead) galaxies the light will be too redshifted for us to detect it. that's the breaks

astronomy peters out