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Abstract

We present the first massive frequency analysis of the 1200 first overtone RR Lyrae stars in the Large Magellanic Cloud observed in the first 4.3 yr of the MACHO project. Besides the many new double-mode variables, we also discovered stars with closely spaced frequencies. These variables are most probably nonradial pulsators.

Type
Part 4. Blazhko Phenomenon
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Alcock, C. et al. 2000, in preparationGoogle Scholar
Dziembowski, W.A. & Cassisi, S. 2000, in these proceedings, p. 321Google Scholar
Moskalik, P. 2000, in these proceedings, p. 313Google Scholar
Olech, A., Kaluzny, J., Thompson, I.B., et al. 2000, in these proceedings, p. 317Google Scholar
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Frequency Analysis of the RRc Variables of the MACHO Database for the LMC
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Frequency Analysis of the RRc Variables of the MACHO Database for the LMC
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Frequency Analysis of the RRc Variables of the MACHO Database for the LMC
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