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Table 3

Program stars with the number of valid observations, whether Hα variability, a single, or double BD; the Ca ii IR triplet is observed; the measured D⋆and λ1, with mean values in case of more than one observation; and stellar parameters.

Star # of obs. Sp Hα Double IR Ca ii D ⋆ λ1 –3700 T eff log gpol vsini
U/V/N Type var? BD? emiss.? [dex] [Å] [K] [dex] [km s-1]
HIP 11116 4/4/4 B8III N N N 0.35 29.97 11 994 3.47 190
HIP 15188 1/1/1 B3: – – N – – – – –
HIP 23161 2/2/2 B7III – N N 0.335 29.97 12 272 3.45 150
HIP 24475 3/4/3 B9II Y N N 0.44 25.50 10 643 3.29 220
HIP 25007 6/6/6 B3IV Y Y N 0.183 38.30 18 089 3.63 –
HIP 25690 4/4/4 A0IV – N N 0.525 50.14 9691 3.70 90
HIP 25950 1/2/0 B7: N – N – – – – –
HIP 26368 2/2/2 A1III N N Y 0.535 45.65 9550 3.57 190
HIP 26964 2/2/1 B4V – Y N 0.262 50.2 15 220 4.00 200
HIP 28561 3/3/3 B8IV Y Y Y 0.399 40.4 11 554 3.73 70
HIP 29635 8/8/9 B8IV N N Y 0.395 41.16 11 409 3.75 230
HIP 31362 1/1/1 B8IV – N N 0.443 38.92 10 769 3.64 270
HIP 32474 10/14/16 A0III Y N N 0.524 44.52 9733 3.60 120
HIP 33509 1/1/1 B4V – Y N 0.226 45.65 15 747 3.92 160
HIP 34144 1/1/1 B8III – N N 0.4 27.73 11 204 3.38 200
HIP 36009 1/1/1 B4V – N N 0.23 50.14 16 435 4.00 40
HIP 37007 6/6/6 B7IV N N Y 0.34 36.68 12 245 3.70 230
HIP 39183 2/2/2 A0III Y N : 0.481 25.50 10 167 3.22 190
HIP 39483 10/11/11 B6IV Y N N 0.28 34.44 13 583 3.60 130
HIP 39595 1/1/1 B9IV – N Y 0.455 38.92 10 592 3.63 240
HIP 41085 1/1/1 B5IV – Y N 0.245 41.16 14 860 3.84 250
HIP 41268 2/2/2 B8III – Y N 0.384 29.97 11 460 3.45 240
HIP 42060 1/1/1 B7V – N N 0.35 45.65 12 235 3.95 250
HIP 43073 1/1/1 B9IV – N N 0.466 38.92 10 413 3.62 250
HIP 43114 1/1/0 B5IV: – N N – – – – –
HIP 44423 2/3/3 B7IV N N N 0.362 38.92 11 909 3.74 160
HIP 46329 2/2/2 B5IV Y N N 0.25 45.65 14 763 3.95 160
HIP 47868 1/1/1 B0III: – N N 0.067 23.70 – – –
HIP 47962 1/3/3 A0IV N N N 0.517 45.65 9786 3.65 220
HIP 48582 4/6/6 B5IV Y Y Y 0.26 51.26 15 396 4.01 –
HIP 48943 2/5/2 B5IV N Y Y 0.284 43.95 14 077 3.81 190
HIP 51444 1/2/2 B5III Y N N 0.23 25.50 14 795 3.30 250
HIP 51491 3/3/4 B9III Y N Y 0.475 38.92 10 341 3.60 230
HIP 51546 2/2/2 A0V: – N N – – – – 210
HIP 52977 21/21/21 B6III Y N N 0.26 34.44 14 076 3.57 200
HIP 56393 1/1/1 A1IV – N : 0.56 52.39 9200 3.62 270
HIP 57861 4/6/6 B6IV Y N N 0.29 38.92 13 390 3.76 270
HIP 59970 2/2/2 A1IV-III – N : 0.574 48.45 – – –
HIP 64501 2/2/2 B8IV – N N 0.39 38.92 11 512 3.77 –
HIP 64867 5/6/6 A0III N N N 0.524 36.68 9708 3.43 170
HIP 66339 1/1/1 B3V – Y N 0.222 52.7 17 493 4.00 210
HIP 66351 2/2/2 B9III – N N 0.469 37.80 10 404 3.57 140
HIP 68100 2/2/2 B6V – N N 0.326 46.77 12 804 3.96 100
HIP 69429 4/6/6 A0IV N N N 0.521 45.65 9749 3.63 190
HIP 71668 3/3/3 B2V: N N N – – – – –
HIP 71974 12/141/4 A0IV N N N 0.522 47.89 9709 3.64 160
HIP 78375 1/1/1 B9: N N : – – – – –
HIP 80577 3/3/3 B8IV Y N N 0.39 47.89 11 472 3.97 100
HIP 80820 3/3/3 B9III Y N N 0.44 25.50 10 576 3.28 150
HIP 81321 0/2/2 A0V: – – N – – – – –
HIP 82874 1/1/0 B7III – N N 0.311 32.20 12 755 3.50 240
HIP 83278 3/3/3 B9IV N N N 0.437 36.68 10 816 3.59 230
HIP 84184 3/3/3 B8IV Y Y N 0.37 38.92 11 808 3.77 270
HIP 85138 14/15/15 B8IV Y N N 0.39 34.44 11 365 3.61 180
HIP 85195 28/29/29 B9III Y N N 0.48 38.92 10 253 3.58 250
HIP 85566 3/3/3 A1III N N : 0.53 38.92 9572 3.45 240
HIP 87032 3/3/3 B8V: N N Y – – – – 300
HIP 87698 1/2/2 A0III N N N 0.523 41.16 9725 3.54 210
HIP 88172 2/5/3 B8IV N N N 0.39 35.56 11 436 3.65 180
HIP 88374 21/25/25 B9IV Y N N 0.445 45.65 10 730 3.84 140
HIP 89486 14/14/15 A0III Y N N 0.51 41.16 9874 3.57 180
HIP 89500 5/5/5 B9III N N N 0.46 29.97 10 443 3.39 240
HIP 90096 4/5/5 B8IV N N N 0.41 36.68 11 170 3.65 200
HIP 90509 2/2/2 B8IV – N : 0.42 38.92 11 062 3.71 250
HIP 91460 3/3/3 A1III N N N 0.54 32.20 9503 3.25 150
HIP 91975 2/3/3 B9III Y N : 0.455 35.56 10 600 3.55 250
HIP 92038 3/3/3 B7III Y Y Y 0.303 32.20 13 002 3.54 170
HIP 93993 3/3/3 A0III N N N 0.524 43.40 9694 3.58 10
HIP 94770 2/2/2 B8IV – N Y 0.41 35.56 11 145 3.60 260
HIP 94859 1/3/3 B7III Y N : 0.33 35.56 12673 3.65 240
HIP 94986 24/36/36 B6III Y N N 0.28 36.68 13 706 3.68 120
HIP 95109 1/2/2 B8V N N N 0.395 49.01 11 518 3.98 260
HIP 96453 1/3/3 B6III Y N N 0.26 29.97 14 172 3.44 230
HIP 99457 7/9/3 B1IV Y N N 0.101 41.16 22 907 3.71 –
HIP 100664 2/3/3 A0III N N N 0.506 36.68 9908 3.47 190
HIP 104508 18/24/24 B9IV Y N N 0.43 36.68 10915 3.61 270
HIP 108022 2/5/5 B6III N N N 0.29 27.73 13 100 3.40 110
HIP 108402 5/5/5 B7V N Y Y 0.391 61.39 12 682 4.03 250
HIP 108597 3/3/3 B5IV N Y Y 0.256 38.92 14 473 3.76 –
HIP 108975 2/2/2 B4IV N N N 0.264 38.65 14 648 3.66 –

Notes. For the double BD and Ca ii flags “Y” and “N” are clear statements, “:” means uncertain, and “–” mean no suitable spectra were available. Newly identified Be stars are indicated in bold face. In case of Hα variability, “–” means that all spectra, even if more than one, were taken on the same night.

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