The CP Stars, an overview: Then and now

Physics

Scientific paper

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Stars: Abundances, Stars: Chemically Peculiar, Stars: Individual: (Vega, Merak, Α And, 32 Aqr, Σ Boo, Κ Cnc, Θ Cyg, Π Dra, 46 Dra, Γ Equ, 112 Her, Φ Her, Υ Her, Θ Leo, Μ Lep, 33 Lib, Χ Lup, 21 Lyn, Σ Ori E, Ι Psc, O Peg, 53 Tau, 68 Tau, 15 Vul, Hr 178, Hr 465, Hr 1728, Hr 1890, Hr 4072, Hr 7143, Hr 7245, Hr 7361, Hr 7664, Hr 7775, Hr 8349, Hd 965, Hd 29647, Hd 101065, Hd 166473, Hd 213637, Hd 215441, Hd 217522).

Scientific paper

We briefly review the traditional classifications of CP stars. The current availability of large numbers of abundances now make it possible to use multivariate techniques, both to supplement traditional classification methods and probe the abundance patterns. We discuss cluster analysis and correlation matrices for sample material. We review the historical resistance to the notion that CP stars were indeed chemically peculiar. Modern work shows that while these objects do indeed have atmospheric anomalies, they are nevertheless chemically peculiar.

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