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

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RR LyraeOld Stars (> 10 Gyr)Horizontal branch starsthat lie in the instabilitystripBurn He in coreIntrinsically variableRadially pulsate Amplitude’s between 0.1and 1 magnitudesPeriods less than a day(Smith 1995)
Bailey Types Based on shape oflight curve RRab pulsate in thefundamental mode RRc pulsate in thefirst overtone RRd stars pulsate ina combination of thefundamental mode &the first overtone
Page 1 and 2: RR Lyrae in LMC Globular Clusters:I
Page 3: MW Inner 100kpc
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 28 and 29: 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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