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Ap and Bp stars are chemically peculiar stars (hence the "p") of spectral types A and B which show overabundances of some metals, such as strontium, chromium, or europium. In addition, larger overabundances are often seen in praseodymium and neodymium. These stars have a much slower rotation than normal for A- and B-type stars, although some exhibit…
Magnetic fields, Abundance spots & Rapidly oscillating Ap stars
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stars field magnetic ap rotation overabundances fields theory high star peculiar exhibit axis variations rotating bp spectral often much normal
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Ap and Bp stars | related to Magnetic fields | Ap | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | Bp | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | B-type | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | HD | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | Typically | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | In | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | This | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | The | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | ISM | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | There | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | Another | 0.60 | section |
| Ap and Bp stars | related to Magnetic fields | A-type | 0.60 | section |
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