Low-dimensional chaos in stellar pulsations

Low-dimensional chaos in stellar pulsations is the current interpretation of an established phenomenon. ^[1]

7 relations: Index of physics articles (L), List of stellar properties, RV Tauri variable, Semiregular variable star, Stellar pulsation, Variable star, W Virginis variable.

Index of physics articles (L)

The index of physics articles is split into multiple pages due to its size.

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List of stellar properties

Pages Related to Stellar properties, Pages using the word stellar in a physics context.

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RV Tauri variable

RV Tauri variables are luminous variable stars that have distinctive light variations with alternating deep and shallow minima.

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Semiregular variable stars are giants or supergiants of intermediate and late spectral type showing considerable periodicity in their light changes, accompanied or sometimes interrupted by various irregularities.

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Stellar pulsation

Stellar pulsations are caused by expansions and contractions in the outer layers as a star seeks to maintain equilibrium.

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Variable star

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) fluctuates.

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W Virginis variable

W Virginis variables are a subclass of Type II Cepheids which exhibit pulsation periods between 10–20 days,Wallerstein, G.,, Publications of the Astronomical Society of the Pacific, 114 p.689–699 (2002) and are of spectral class F6 – K2.

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Low dimensional chaos in stellar pulsations.

References

[1] https://en.wikipedia.org/wiki/Low-dimensional_chaos_in_stellar_pulsations

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