  This project aims to image a subset of galaxies in the nearby group Eridanus
in HI emission and in radio continuum using the GMRT. The typical resolution of
HI images will be $\sim$1 kpc with a 3$\sigma$ sensitivity to HI mass of a few
times 10$^{7}$ M$_\odot$. The rotation curves obtained using the HI velocity
field together with the 2MASS magnitudes in the near infrared will be used to
construct the Tully-Fisher relation for this group. High resolution (sub-kpc)
multi-frequency radio continuum images will be used to study star-formation
rates, radio morphologies and spectral indices of Eridanus galaxies. About half
of the galaxies have already been observed and further observations on some
late type galaxies are proposed with the GMRT. We present here the HI image and
the rotation curve for a member of this group viz. NGC 1385.
