  We analyzed the eclipse light curve of the nova-like star RW Tri in its low
luminosity state. During approximately 150 days, RW Tri was about one magnitude
fainter than in its usual state. Our eclipse map shows that the brightness
temperature in the disc ranges from 19000 K near the white dwarf to 8700 at the
disc edge. For the inner parts of accretion disc, the radial temperature
distribution is flatter than that predicted from the steady state models, and
for the outer parts, it is close to the R^(-3/4) law. Fitting of the
temperature distribution with one for the steady state disc model gives a mean
accretion rate of (3.85+-0.19) 10^{-9} M year^(-1). The hotspot in the disc is
placed at a distance of 0.17a from the white dwarf, where a is the orbital
separation.
