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- W189260060 abstract "Rapidly oscillating Ap (roAp) stars are cool magnetic Ap SrCrEu stars which pulsate in high-overtone ( n ≫ l ), low-degree (ℓ ≤ 3) p -modes, with periods from 6 to 15 minutes and typical amplitudes of a few millimagnitudes. 28 such stars are currently known. The roAp phenomenon is confined to a well-defined region of the Strömgren photometry parameter space. However, this region also contains other Ap stars, in which no pulsation could be detected, despite sometimes thorough searches. These apparently constant Ap stars (non-oscillating Ap stars, or noAp stars) appear remarkably similar to the roAp stars in many respects (e.g. colour indices, abundances, magnetic fields). Here we present recently found indications for differences between both groups." @default.
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- W189260060 date "1998-01-01" @default.
- W189260060 modified "2023-09-24" @default.
- W189260060 title "The Single Life of Rapidly Oscillating Ap Stars" @default.
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- W189260060 doi "https://doi.org/10.1017/s0074180900238837" @default.
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