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In the first paper of this series we used HI observations of the 19 brightestspirals in Coma to analyze the dynamical state of the cluster. In this paper wepresent the detailed HI distribution and kinematics of the spirals that weredetected in HI, and radio continuum data for a sample of star forming and poststarburst galaxies in Coma. We discuss the importance of ICM-ISM interactionsto explain the observed HI morphology. A rough comparison of observed HI sizeswith predicted HI sizes from simulations by Abadi et al. (1999) givesreasonable agreement. We use the results on radio continuum emission toestimate the star formation rate in the PSB galaxies we pointed at. The radiocontinuum emission in the 11 so called post starburst galaxies, identified byCaldwell et al. (1993) in the cluster, is weak. Eight of the 11 were notdetected down to a 3 sigma upper limit of 0.6 mJy. This sets an upper limit tothe star formation rate in these galaxies of less than 0.2 solar masses peryear. The three detected post starburst galaxies have a star formation rate ofless than one solar mass per year. Thus none of the post starburst galaxies inComa are dust enshrouded starbursts.Comment: Accepted by Astronomy & Astrophysics; 17 pages and 31 figure

VLA HI Imaging of the brightest spiral galaxies in Coma