Concept information
Preferred term
Semi-regular variable stars
Definition
- A type of giant or supergiant pulsating variable star, with intermediate or late spectra, showing noticeable periodicity in its light changes, accompanied or sometimes interrupted by various irregularities. Periods lie in the range from 20 to more than 2000 days, while the shapes of the light curve may be rather different and variable with each cycle. The amplitudes may be from several hundredths to several magnitudes (usually 1-2 magnitudes in the V filter). Examples are Betelgeuse, Antares, and Rasalgethi. Semiregular variables are classified in several subtypes: SRA, SRB, SRC, and SRD. (en)
Broader concept
Narrower concepts
- SRa variable stars (en)
- SRb variable stars (en)
- SRc variable stars (en)
- SRd variable stars (en)
- SRS variable stars (en)
Entry terms
- Semiregular variable stars (en)
Example
- Betelgeuse (en)
URI
http://astrothesaurus.org/uat/1444
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