RR Lyrae in LMC Globular Clusters: Insights into the Oosterhoff ...

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Trends in Fourier Parameters vs Cluster Metallicity for RRab stars in Globular Clusters. Data from Lázaro etal. (2006), Arellano Ferro et al. (2008), Contreras et al. (2010), Zorotovic et al.(2009), Soszyński et al. (2009), Kuehn et al. (2010).
Trends in Fourier Parameters magnitude vs Cluster Metallicity for RRab stars in Globular Clusters. Data fromLázaro et al. (2006), Arellano Ferro et al. (2008), Contreras et al. (2010), Zorotovic etal. (2009), Soszyński et al. (2009), Kuehn et al. (2010).
Page 1 and 2: RR Lyrae in LMC Globular Clusters:I
Page 3 and 4: MW Inner 100kpc
Page 5 and 6: Bailey Types Based on shape oflight
Page 7 and 8: The Oosterhoff dichotomy poses stro
Page 10 and 11: Target Objects 5 LMC globular clust
Page 14 and 15: NGC 1466 Periods accurate to betwee
Page 16 and 17: NGC 1466
Page 18 and 19: Reticulum Previously searched by Wa
Page 20 and 21: Other Clusters3 clusters included i
Page 22 and 23: Fourier Fits
Page 24 and 25: Fourier Derived Parameters RRab sta
Page 26 and 27: Trends in Fourier Parameters vs Clu
Page 30 and 31: Summary The processes that created
Page 32 and 33: Are All Oo-Int Systems Equal?Draco

RR Lyrae in LMC Globular Clusters: Insights into the Oosterhoff ...

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