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RR Lyrae - Wikipedia, the free encyclopedia
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RR Lyrae variable - Wikipedia, the free encyclopedia
RR Lyrae variables are periodic variable stars, commonly found in globular clusters, and often used as standard candles to measure galactic distances. This type of variable is named after the prototy...
en.wikipedia.org/wiki/RR_Lyrae_variable |
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RR Lyrae is the prototype of a class of variables (that is, the ‘main’ star in that category, usually the first star discovered with its particular characteristics). RR Lyrae variables are very old giants which pulsate (that is their outer layer expands and contracts).
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Hutchinson encyclopedia article about RR Lyrae. RR Lyrae. Information about RR Lyrae in the Hutchinson encyclopedia. ... W Virginis stars are sometimes called Type II Cepheids, while RR Lyrae stars are Cepheidlike variables with periods that fall in the range 0.3 and 0.7 days. They are sometimes described as cluster...
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RR Lyrae stars: the GEOS maxima database ... It is then important to monitor the period variations of RR Lyraes to make a catalogue of their behavior to help understanding the phenomenon as V.P. Tsesevich ("RR Lyrae stars", 1969, Israel program for scientific translation, for the english translation) made in a first...
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GEOS RR Lyr database ... GEOS RR Lyr Survey ... The GEOS RR Lyr database is intended to help observations and studies on RR Lyr stars. It contains times of light maximum of RR Lyr stars obtained either visually or with electronic devices or photographically.
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Summary The student finds the distance to the globular cluster, Messier 4 (M4), using observations of an RR Lyrae star and the mean absolute magnitude of RR Lyrae variables. Background and Theory; As stars evolve, their atmospheres become unstable and the star becomes intrinsically variable.
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