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Table 2

Adopted and calculated parameters for the sample of Be stars with emission in the Brγ line.

Name HD number mKa STa db Teffc V sin ic Vcc Pd Re e
(mag) (pc) (K) (km s−1) (km s−1) (°) (R)
η Tau HD 23630 2.940 B7III 127 ± 8f 12 258 ± 505 149 ± 8 274 ± 15 34 6.6 0.71
28 Tau HD 23862 4.937 B8Vne 117 ± 5 12 106 ± 272 290 ± 15 420 ± 22 69 3.5 0.19
28 Eri HD 28497 5.798 B2(V)ne 465 ± 63 26 724 ± 427 342 ± 24 631 ± 45 120 4.1 0.63
56 Eri HD 30076 5.452 B2(V)nne 822 ± 486f 20 488 ± 330 225 ± 12 456 ± 25 148 11.0 0.47
105 Tau HD 32991 4.775 B2Ve 250 ± 43f 20 900e 175 ± 18g 126 3.8 0.90
ψ01 Ori HD 35439 5.355 B1Vn 318 ± 85 22 134 ± 665 266 ± 13 513 ± 26 142 6.1 0.09
120 Tau HD 36576 4.777 B2IV-Ve 476 ± 73 22 618 ± 508 266 ± 13 487 ± 25 113 4.5 0.87
ζ Tau HD 37202 2.970 B1IVe-shell 136 ± 16 19 310 ± 550 326 ± 7 466 ± 13 34 6.1 0.58
ω Ori HD 37490 4.805 B3Ve 423 ± 52 14 492e 155 ± 5h 319h 9 13.5 0.02
V696 Mon HD 41335 4.770 B3/5Vnne 403 ± 122 20 902 ± 610 376 ± 26 520 ± 36 147 8.2 0.44
β01 Mon HD 45725 4.030 B4Ve-shell 207 ± 49 17 810 ± 455 345 ± 21 486 ± 30 14 5.0 0.32
OW Pup HD 60606 5.050 B2Vne 363 ± 32 18 030 ± 332 285 ± 16 441 ± 25 6.2 0.56
V374 Car HD 66194 5.359 B3Vn 379 ± 47f 14 089e 200 ± 29h 367h 130 7.9 0.32
MX Pup HD 68980 4.554 B2ne 284 ± 13 25 126 ± 642 152 ± 8 534 ± 31 6.0 0.40
o Aqr HD 209409 4.661 B7IVe 133 ± 4 12 942 ± 402 282 ± 20 391 ± 27 6 4.4 0.17
31 Peg HD 212076 4.685 B2IV-Ve 497 ± 70 19 270 ± 326 103 ± 6 439 ± 26 58 8.0 0.70
π Aqr HD 212571 5.351 B1III-IVe 239 ± 16 26 061 ± 736 233 ± 15 558 ± 37 177 5.2 0.30
ϵ PsA HD 214748 4.400 B8Ve 149 ± 15 11 966 ± 356 205 ± 13 317 ± 21 3 6.6 0.02

Notes. Values taken from: (a)CDS database; (b) van Leeuwen (2007), except noted otherwise; (c)Frémat et al. (2005), except notedotherwise; (d)Yudin (2001); (e) SED fittings; (f) Astraatmadja & Bailer-Jones (2016); (g)Abt et al. (2002); (h)Chauville et al. (2001).

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