Table 2
Ap stars with resolved magnetically split lines: stars with magnetic measurements from the literature.
| HD/HDE | Other id. | V | Sp. type | Ref. | Period | Ref. | HJD0 | Phase origin | Ref. |
|
|
|||||||||
| 3988 | CPD −83 10 | 8.351 | A0p CrEuSr | 1 | |||||
| 18610 | CPD −73 195 | 8.162 | A2p CrEuSr | 2 | |||||
| 33629 | CoD −33 2151 | 9.064 | A9p SrCr | 3 | |||||
| 42075 | CoD −26 2736 | 8.968 | A5p EuCrSr | 3 | |||||
| 44226 | CoD −25 3118 | 9.492 | A5p SrEuCr | 3 | |||||
| 46665 | BD −22 1450 | 9.441 | A0p SrEu | 3 | |||||
| 47009 | BD −13 1560 | 9.070 | A0p EuCr | 3 | |||||
| 52847 | BD −22 1666 | 8.157 | A0p CrEu | 3 | |||||
| 55540 | BD −20 1779 | 9.498 | A0p EuCr | 3 | |||||
| 57040 | CPD −53 1304 | 9.207 | A2p EuSr | 1 | 13 474 |
1 | |||
| 61513 | CoD −29 4702 | 10.161 | A0p CrEuSr | 1 | |||||
| 66318 | CPD −60 1017 | 9.665 | A0p EuCrSr | 4 | |||||
| 69013 | BD −15 2337 | 9.456 | A2p SrEu | 3 | |||||
| 70702 | CoD −51 2962 | 8.572 | B9p EuCrSr | 1 | |||||
| 72316 | CoD −33 5118 | 8.804 | Ap CrEu | 3 | |||||
| 75049 | CoD −50 3542 | 9.090 | A0p EuCrSi | 3 | 4048267 |
5 | 2 454 509.550 | ⟨ Bz ⟩ max. | 6 |
| 76460 | CPD −61 1106 | 9.805 | A3p Sr | 1 | |||||
| 81588 | CoD −47 4913 | 8.445 | A5p SrCrEu | 1 | |||||
| 88241 | CoD −39 6174 | 7.920 | F0p SrEu | 1 | |||||
| 88701 | CoD −36 6209 | 9.258 | B9p CrEu | 3 | 25765 |
3 | |||
| 92499 | CoD −42 6407 | 8.890 | A2p SrEuCr | 7 | >5 yr? | 3 | |||
| 96237 | CoD −24 9514 | 9.434 | A4p SrEuCr | 3 | 2091 |
3 | |||
| 97394 | CoD −42 6806 | 8.797 | A5p EuCrSr | 8 | |||||
| a | BD + 0 4535 | 9.92 | Ap SrEu | 9 | |||||
| 110274 | CoD −58 4688 | 9.328 | A0p EuCr | 3 | 2653 |
3 | |||
| 117290 | CoD −48 8252 | 9.281 | A3p EuCrSr | 3 | >5.7 yr? | 3 | |||
| 121661 | CPD −62 3790 | 8.556 | A0p EuCrSi | 3 | 470 |
3 | |||
| 135728 | CoD −30 12099 | 8.602 | A2p SrEuCr | 3 | |||||
| 143487 | CoD −30 12753 | 9.420 | A3p SrEuCr | 3 | |||||
| 154708 | CPD −57 8336 | 8.744 | A2p SrEuC | 10 | 5363 |
11 | 2 454 257.740 | ⟨ Bz ⟩ max. | 12 |
| 157751 | CoD −33 12069 | 7.674 | B9p SiCr | 7 | |||||
| 158450 | BD −7 4448 | 8.514 | A0p SrCrEu | 1 | 8524 |
1 | |||
| 162316 | CPD −75 1401 | 9.338 | A3p SrEu | 1 | 9304 |
1 | |||
| 168767 | CD −26 13084 | 8.674 | A0p EuCr | 1 | |||||
| 177268 | CD −34 13384 | 9.034 | A2p CrEu | 1 | |||||
| 178892 | BD + 14 3811 | 9.27 | B9p SrCrEu | 13 | 82478 |
13 | 2 452 708.562 | max. brightness in V | 13 |
| 179902 | BD −21 5306 | 10.35 | A1p SrCrEu | 1 | |||||
| 184120 | BD −20 5601 | 10.220 | A0p CrEu | 1 | |||||
| 185204 | CD −47 13020 | 9.534 | A2p SrEuCr | 1 | |||||
| 191695 | BD −21 5644 | 7.010 | A3p SrEuCr | 1 | |||||
| 215441 | BD + 54 2846 | 8.851 | B9p Si | 14 | 9487574 |
15 | 2 448 733.714 | max. brightness in B | 15 |
Notes. HJD0 and the phase origin information appear only when available in the literature. In particular, Freyhammer et al. (2008) and Elkin et al. (2012) used photometric databases to obtain reliable period determinations, but they give no indication about the phasing of the data.
Reference. (1) Elkin et al. (2012); (2) Stütz et al. (2003); (3) Freyhammer et al. (2008); (4) Bagnulo et al. (2003); (5) Kochukhov et al. (2015); (6) Elkin et al. (2010c); (7) Hubrig & Nesvacil (2007); (8) Elkin et al. (2011) (9) Elkin et al. (2010b); (10) Hubrig et al. (2005); (11) Landstreet et al. (2014); (12) Hubrig et al. (2009a); (13) Ryabchikova et al. (2006); (14) Babcock (1960); (15) North & Adelman (1995).
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