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We present deep single-dish HI observations of a sample of six nearby E+Agalaxies (0.05<z<0.1). A non-negligible fraction of a local sample of E+As aredetected in HI. In four galaxies, we have detected up to a few times 10^9 Msunof neutral gas. These E+A galaxies are almost as gas-rich as spiral galaxieswith comparable luminosities. There appears to exist no direct correlationbetween the amount of HI present in an E+A galaxy and its star-formation rateas traced by radio continuum emission. Moreover, the end of the starburst doesnot necessarily require the complete exhaustion of the neutral gas reservoir.Most likely, an intense burst of star formation consumed the dense molecularclouds, which are the sites of massive star formation. This effectively stopsstar formation, even though copious amounts of diffuse neutral gas remain. Theremaining HI reservoir may eventually lead to further episodes of starformation. This may indicate that some E+As are observed in the inactive phaseof the star-formation duty cycle.Comment: Accepted for publication in ApJ, 9 pages, 3 figures (reduced in  resolution

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