MULTICOLOR PHOTOMETRY OF LONG PERIOD VARIABLES
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UNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
Abstract
Multicolor photometry is made of sixty seven late type stars over wavelengths ranging from 0.3µ to 10.2µ. The observations enable one to distinguish between classes M, S and C. The M and S stars unreddened by interstellar extinction can be separated and t
