  We present recent polarimetric results of magnetically active late-type
dwarfs. The polarization in these stars is found to be wavelength dependent,
decreasing towards the longer wavelength. The average values of degree of
polarization in these active dwarfs are found to be 0.16+/-0.01, 0.080+/-0.006,
0.056+/-0.004 and 0.042+/-0.003 per cent in B, V, R, and I bands, respectively.
Present results indicate that polarization in the majority of active dwarfs are
primarily due to sum of the polarization by magnetic intensification and
scattering. However, supplementary sources of the polarization are also found
to be present in some active stars. The correlations between the degree of
polarization and various activity parameters like Rossby number, chromospheric
activity indicator and coronal activity indicator are found to be stronger in B
band and weaker in I band.
