...NGC 128

Based on observations taken at ESO La Silla and at the Special Astrophysical Observatory (SAO) of the Russian Academy of Sciences (RAS).

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

...(5.4 kpc)

We assume throughout the paper a distance of 56 Mpc for the galaxy and H₀ = 75 km s$^{-1}~{\rm Mpc}^{-1}$.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

...1993)

The error on the total luminosity does not take into account the error on the adopted distance of the galaxy.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.