H-alpha and H-beta are different emission lines of hydrogen - ie UV light from a star excites hydrogen atoms electrons - when these excited electrons return to their base state they release photons on the way down. Emission nebulae, since they are mostly composed of hydrogen, are rich in the hydrogen emissions.....
The filters have a "bandpass" which refers to the width of the band of light allowed - ie which wavelengths - a common one is a 13nm Ha filter - lets through only a 13nm band of light centred on the wavelength below.
H-alpha - 656.3nm (red light)
H-beta - 486.1nm (blue-green light)
http://en.wikipedia.org/wiki/H-alpha
UV/IR filters block the non-visible light regions at either end of the visible spectrum (UV below around 380nm, IR above about 750nm).... helps avoid star bloat from IR mainly.....
The beauty of this for us is exclusion of the major light pollution emission (sodium/mercury vapour lights) and little moon light.