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RR Lyrae variables

Published online by Cambridge University Press:  25 May 2016

G. Bono  and
M. Marconi
G. Bono
Affiliation:
Trieste Astronomical Observatory, Via G.B. Tiepolo 11, 34131 Trieste, Italy, bono@oat.ts.astro.it
M. Marconi
Affiliation:
Dept. of Physics, Univ. of Pisa, Piazza Torricelli 2, 56100, Pisa, Italy, marcella@astr1pi.difi.unipi.it

Extract

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On the basis of a historical overview we outline the relevant results which allowed to approach on firm basis the physical mechanisms which govern the radial pulsation of RR Lyrae variables, revealing the astrophysical parameters which account for their limiting amplitude pulsational behavior.

Type
Stellar Oscillations and Pulsations
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 305 - 310
Copyright
Copyright © Kluwer 1997 

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