I'm not sure if this will help for intuition behind deriving the Gaussian Distribution, but here's the reason why it follows from the binomial distribution:
Think of a collection of an infinite number of particles distributed throughout space. The Gaussian Distribution can be thought of as randomly choosing n particles out of the infinitely many. What we are interested in (for now) is the expected total thermal energy in the system of n particles chosen randomly, or at least the distribution of chance that a collection of n particles will have a particular thermal energy.
After doing this a few times, we find the average thermal energy for a collection of "n" particles to be E, which we can now take to be constant (think of this stage as being something like an induction hypothesis: we can use this to determine how the energy is distributed later).
We can now look at how that total energy E is distributed within the system of n particles:
create a "histogram" of possible thermal energies for the n particles, with bin width of "e". The histogram sorts particles within the system of n particles: each "bin" bi will contain ni particles, so that [tex]\sum[/tex]ni = n.
You can imagine that when you give a certain total energy to the system of n particles, we can (with a few assumptions) create a finite number of energy distributions within the n particles that allow the system to have energy E.
Count unique configurations for every allowable energy value (k*e) to get the binomial distribution as a function of energy level. (for the "0" state, all the particles are in the lowest bin: this is 1 configuration; for the "1" state, one particle is in the 1st energy level while the rest are in the lowest bin: this gives n configurations; etc.).
Here are variables to consider:
The average energy density of particles around the n particles chosen (this gives you the amount of energy you have to work with within the system of n particles).
The (classical) fact that you can choose an energy partition e(E), so that there will be an equal number of particles as there are energy "bins" (you then proceed to take the limit as n and e go to infinity and 0 respectively: with the preceding assumption, e = E/n, where E is the "total energy" of the system given by the average energy density) .