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Multiperiodicity in pulsating red giants
Published online by Cambridge University Press: 12 April 2016
Abstract
We describe several aspects of the variability of bright pulsating red giant (PRG) stars, with emphasis on the determination of pulsation modes and pulsation masses by using observed multiperiodicity and pulsation constants (Q- values). Our studies of bright PRGs provide a model for the analysis and interpretation of the thousands of PRGs being discovered in surveys of Local Group galaxies.
- Type
- Part 5. Red Giants, Miras, post-AGB stars and proto-planetary nebulae
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 348 - 352
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
- 2
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