ABSTRACT. It is widely believed that Sciama's (1990) decaying-neutrino theory has been disproved by the failure of Davidsen et al. ( 1991 ) to detect an unidentified emission line at ~ 15 eV (in the rest frame) from the dark matter in the cluster of galaxies A665 (e.g., Trimble 1992). Here we show that recent X-ray data for A665 favor models in which the dark matter in the regions of the cluster observed by Davidsen et al. is mainly baryonic. Thus the decaying-neutrino theory continues to be viable.