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The pulsating variables can be further divided into the following subclasses: short-term, long-term, semiregular, and irregular. Short-term variables have well-defined periods ranging from less than one day to more than 50 days. The long-term variables are the most numerous of all pulsating stars. They are red giant and supergiant stars with periods ranging from a few months to more than a year. Semiregular variables are stars whose periodic variations are occasionally interrupted by sudden bursts of light. Irregular variables show no periodicity in their variations in brightness. The amplitude of their fluctuations in brightness is in general smaller than the fluctuations of the long-term regular variables.
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