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What (who) is long-period stability - definition
DESCRIPTION FOR CERTAIN COOL LUMINOUS PULSATING VARIABLE STARS
Long-Period Variable Star; Long-period variables; Long period variable; Long period variables; Long-period variable stars; Long period variable star; Long period variable stars; Long-period-variable stars; Long-period-variable star; Long-period-variable; Long-period-variables; LPV star; LPV stars; Long-period variable; OGLE small amplitude red giant
![Light curves of four [[Mira variable]]s in the [[galaxy]] [[Centaurus A]]](https://commons.wikimedia.org/wiki/Special:FilePath/Eso0315i.jpg?width=200 "Light curves of four [[Mira variable]]s in the [[galaxy]] [[Centaurus A]]")
Long-period variable star
The descriptive term long-period variable star refers to various groups of cool luminous pulsating variable stars. It is frequently abbreviated to LPV.
Secondary stability
BOAT'S ABILITY TO RIGHT ITSELF
Secondary Stability; Draft:Secondary Stability
Secondary stability, also known as reserve stability, is a boat or ship's ability to right itself at large angles of heel (lateral tilt), as opposed to primary or initial stability, the boat's tendency to stay laterally upright when tilted to low (http://newboatbuilders.com/docs/stability.
BIBO stability
PROCESS CONTROL THEOREM
Bounded-input, bounded-output stability; Bonded-input, bonded-output stability; Bonded-input, bounded-output stability; Bibo stability; BIBO stable
In signal processing, specifically control theory, bounded-input, bounded-output (BIBO) stability is a form of stability for signals and systems that take inputs. If a system is BIBO stable, then the output will be bounded for every input to the system that is bounded.
Wikipedia
Long-period variable star
The descriptive term long-period variable star refers to various groups of cool luminous pulsating variable stars. It is frequently abbreviated to LPV.
