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

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Reticulum Previously searched by Walker (1992)WalkerKuehnRR ab 22 22RR c 10 9RR cand 1 Includes all RR Lyrae found by Walker Ripepi et al. (2004) found 4 possible RRd stars, havenot checked ours yet for double-modes
Reticulum [Fe/H] = -1.66 = 0.552 days = 0.339 days N c /N RRL = 0.31 All suggest Reticulum is an Oosterhoff Iobject
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 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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