The Stark broadening tables for hydrogen Lyman, Balmer and Paschen lin
es published in the early seventies give accurate results for the widt
hs of the beta lines down to relatively low electron densities, and fo
r the far line wings in general. However, the half-widths of the alpha
lines can be in error by as much as a factor of 30, particularly at i
ntermediate densities. Modem theoretical methods are capable of produc
ing accurate values over the entire density range. Recent developments
in the Stark broadening of non-hydrogenic species are also considered
.