R. Nesci, Gianni Rocchi INAFIAPS-Roma, Gruppo Astrofili Monte Subasio
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Abstract
We reobserved in the RC and i(Sloan) bands, during the years 2020-2021, seven Mira variables in Cassiopeia, for which historical i(Sloan) light curves were available from Asiago Observatory plates taken in the years 1967-84. The aim was to check if any of
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