Table 1
Stellar properties for the complete Ap sample, with Teff and L derived from Kochukhov & Bagnulo (2006).
| # | HD | B | V | Sp. type | Teff [K] | L [L⊙] |
|---|---|---|---|---|---|---|
| 1 | 4778 | 6.16 | 6.15 | A3Vp | 9980 | 32.4 |
| 2 | 24712(a) | 6.00 | 6.32 | A9p | 7190 | 7.4 |
| 3 | 108662 | 5.18 | 5.2 | A0p | 10 500 | 64.6 |
| 4 | 108945 | 5.47 | 5.4 | A2pv | 8950 | 51.3 |
| 5 | 118022(b) | 4.94 | 4.96 | Ap | 9060 | 28.8 |
| 6 | 120198 | 5.66 | 5.7 | B9pe | 10 540 | 44.7 |
| 7 | 128898(c) | 3.19 | 3.43 | A7p | 7670 | 11.0 |
| 8 | 137909(d) | 3.68 | 3.97 | F2p | 7430 | 27.5 |
| 9 | 153882 | 6.26 | 6.3 | B9p | 9730 | 100 |
| 10 | 176232(e) | 5.89 | 6.14 | A7p | 7930 | 20.9 |
| 11 | 188041(f) | 5.81 | 5.6 | A5p | 8430 | 35.5 |
| 12 | 201601(g) | 4.68 | 4.94 | A9p | 7620 | 12.6 |
| 13 | 204411(f) | 5.37 | 5.3 | A4pv | 8750 | 89.1 |
| 14 | 220825 | 4.94 | 4.9 | A2pv | 9080 | 22.4 |
Notes. The objects previously observed are in italics, and the corresponding references are given in the Notes.
References.(a) Perraut et al. (2016); (b) Perraut et al. (2015); (c) Bruntt et al. (2008); (d) Bruntt et al. (2010); (e) Perraut et al. (2013); (f) Romanovskaya et al. (2019b); (g)Perraut et al. (2011).
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