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Table 4.
Ap stars with accurately determined rotation periods longer than 1000 d.
HD | Other ID | Sp. type | Prot | Ref. | ⟨Bz⟩rms | B0 | ⟨Bz⟩rms/B0 | q | r | Notes |
---|---|---|---|---|---|---|---|---|---|---|
(d) | (G) | (G) | ||||||||
50169 | BD −1 1414 | A3p SrCrEu | 10 600 | 1 | 1294 | 5076 | 0.25 | 1.43 | −0.96 | SB1 |
9996 | HR 465 | B9p CrEuSi | 7937 | 2 | 713 | – | – | – | −0.35 | SB1 |
965 | BD −0 21 | A8p SrEuCr | 6030 | 3 | 775 | 4253 | 0.18 | 1.00 | −0.50 | |
166473 | CoD −37 12303 | A5p SrEuCr | 3836 | 4 | 1682 | 7131 | 0.24 | 1.52 | −0.99 | roAp |
94660 | HR 4263 | A0p EuCrSi | 2800 | 5 | 1911 | 6232 | 0.31 | 1.06 | 0.92 | SB1 |
187474 | HR 7552 | A0p EuCrSi | 2345 | 6 | 1470 | 5417 | 0.27 | 1.27 | −0.98 | SB1 |
59435 | BD −8 1937 | A4p SrCrEu | 1360 | 7 | – | 3036 | – | 1.87 | – | SB2 |
18078 | BD +55 726 | A0p SrCr | 1358 | 8 | 692 | 3450 | 0.20 | 1.81 | −0.92 | SB1 |
References. (1) Mathys et al. (2019b); (2) Bychkov et al. (2012); (3) Mathys et al. (2019a); (4) this paper; (5) Mathys (2017); (6) Mathys (1991); (7) Wade et al. (1999); (8) Mathys et al. (2016).
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