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The photospheric optical spectra of SN 1994 I obtained with the 2.16 m telescope of Beijing Observatory, show the same features of type-I supernova as in SN 1987 M. The April 10 spectrum is fitted with a Monte Carlo synthesis code. With the abundances of Nomoto et al. and an altered W7 density structure, a reasonable fit is obtained. We find a photospheric velocity of 10 4 km/s, a blackbody...
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