MULTICOLOR PHOTOMETRY OF LONG PERIOD VARIABLES

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UNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX

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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

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