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Table 1

Ap stars with resolved magnetically split lines: stars for which new measurements of the mean magnetic field modulus are presented in this paper.

HD/HDE Other id. V Sp. type Period Ref. HJD0 Phase origin Ref.
965 BD −0 21 8.624 A8p SrEuCr >13 yr 1
2453 BD + 31 59 6.893 A1p SrEuCr 521 d 2 2 442 213.000 ⟨ Bz ⟩ min.
9996 HR 465 6.376 B9p CrEuSi 7936.5 d 3 2 433 301.360 ⟨ Bz ⟩ min. 3
12288 BD + 68 144 7.750 A2p CrSi 349 4 2 448 499.870 ⟨ B ⟩ max. 4
14437 BD + 42 502 7.261 B9p CrEuSi 2687 4 2 448 473.846 ⟨ Bz ⟩ max. 4
18078 BD + 55 726 8.265 A0p SrCr 1358 d 5 2 449 930.000 ⟨ B ⟩ max. 5
29578 CPD −54 685 8.495 A4p SrEuCr ≫5 yr
47103 BD + 20 1508 9.148 Ap SrEu
50169 BD −1 1414 8.994 A3p SrCrEu ≫8 yr
51684 CoD −40 2796 7.950 F0p SrEuCr 371 d 2449947.000 ⟨ B ⟩ max.
55719 HR 2727 5.302 A3p SrCrEu ≫10 yr
59435 BD −8 1937 7.972 A4p SrCrEu 1360 d 6 2 450 580.000 ⟨ B ⟩ max. 6
61468 CoD −27 4341 9.839 A3p EuCr 322 d 2 450 058.500 ⟨ B ⟩ max.
65339 53 Cam 6.032 A3p SrEuCr 802681 7 2 448 498.186 positive crossover 7
70331 CoD −47 3803 8.898 B8p Si 19989 or 19909 2446987.100 arbitrary
75445 CoD −38 4907 7.142 A3p SrEu 6291? 2 449 450.000 arbitrary
81009 HR 3724 7.200 A3p CrSrSi 33984 8 2 444 483.420 max. brightness in v 8
93507 CPD −67 1494 8.448 A0p SiCr 556 d 2 2 449 800.000 ⟨ B ⟩ min. 2
94660 HR 4263 6.112 A0p EuCrSi 2800 d 2 447 000.000 ⟨ B ⟩ min.
110066 HR 4816 6.410 A1p SrCrEu 4900: d 9
116114 BD −17 3829 7.026 F0p SrCrEu 2761 2 447 539.000 ⟨ B ⟩ min.
116458 HR 5049 5.672 A0p EuCr 14839 2 448 107.000 ⟨ Bz ⟩ max.
119027 CoD −28 10204 1 0.027 A3p SrEu
126515 BD + 1 2927 7.094 A2p CrSrEu 12995 2 2 437 015.000 ⟨ B ⟩ max. 10
134214 BD −13 4081 7.467 F2p SrEuCr
137909 β CrB 3.900 A9p SrEuCr 184868 11 2 434 204.700 ⟨ Bz ⟩ pos. extr. 11
137949 33 Lib 6.659 F0p SrEuCr 5195: d 2 453 818.000 ⟨ Bz ⟩ max.
142070 BD −0 3026 7.966 A0p SrCrEu 33718 2 449 878.200 ⟨ Bz ⟩ max.
144897 CoD −40 10236 8.600 B8p EuCr 4857 2 449 133.700 ⟨ B ⟩ min.
150562 CoD −48 11127 9.848 A5p EuSi? ≳ 4.5 yr
318107 CoD −32 13074 9.355 B8p 97088 12 2 448 800.000 ⟨ B ⟩ max.
165474 HR 6758B 7.449 A7p SrCrEu ≫ 9 yr
166473 CoD −37 12303 7.953 A5p SrEuCr ≳10 yr 13
177765 CoD −26 13816 9.155 A5p SrEuCr ≫5 yr
187474 HR 7552 5.321 A0p EuCrSi 2345 d 14 2 446 766.000 ⟨ Bz ⟩ pos. extr. 15
188041 HR 7575 5.634 A6p SrCrEu 22378 2 432 323.000 ⟨ Bz ⟩ min. 16
192678 BD + 53 2368 7.362 A2p Cr 64193 17 2 449 113.240 ⟨ B ⟩ max. 18
335238 BD + 29 4202 9.242 A1p CrEu 4870 2 447 000.000 arbitrary
200311 BD + 43 3786 7.708 B9p SiCrHg 520084 19 2 445 407.513 ⟨ Bz ⟩ pos. extr. 19
201601 γ Equ 4.700 A9p SrEu ≳97 yr 20
208217 CPD −62 6281 7.196 A0p SrEuCr 844475 21 2 447 028.000 ⟨ Bz ⟩ pos. extr.
213637 BD −20 6447 9.611 F1p EuSr >115 d?
216018 BD −12 6357 7.623 A7p SrEuCr ≫6 yr?

Reference. (1) Romanyuk et al. (2014); (2) Mathys et al. (1997); (3) Metlova et al. (2014); (4) Wade et al. (2000c); (5) Mathys et al. (2016); (6) Wade et al. (1999); (7) Hill et al. (1998); (8) Adelman (1997); (9) Adelman (1981); (10) Preston (1970); (11) Kurtz (1989); (12) Bailey et al. (2011); (13) Mathys et al. (2007); (14) Mathys (1991); (15) Landstreet (unpublished; cited by Mathys 1991); (16) Wolff (1969b); (17) Adelman (2006); (18) Wade et al. (1996a); (19) Wade et al. (1997); (20) Bychkov et al. (2016); (21) Manfroid & Mathys (1997).

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