Table 1
Fundamental parameters for the programme’s Be stars.
| HD | Name | ST(a) | LC (a) | V sin i(b) [km s−1] | Teff (b) [K] | log g(b) [dex] |
|---|---|---|---|---|---|---|
| HD 20336 | BK Cam | B2.5 | V | 341 ± 23 | 18 684±517 | 3.865±0.072 |
| HD 23862 | 28 Tau | B8 | V | 290 ± 15 | 12 106 ± 272 | 3.937 ± 0.052 |
| HD 25940 | 48 Per | B3 | V | 220 ± 13 | 16258 ± 582 | 3.572 ± 0.084 |
| HD 28497 | 228 Eri | B2 | V | 342 ± 24 | 26 724 ± 427 | 4.200 ± 0.046 |
| HD 29441 | V1150 Tau | B2.5 | V | 274 ± 42(c) | 18 000(g) | 3.8 (g) |
| HD 32991 | 105 Tau | B2 | V | 175 ± 18(d) | 20900(h) | 3.77(h) |
| HD 35439 | ψ01 Ori | B1 | V | 266 ± 13 | 22 134 ± 665 | 3.920 ± 0.087 |
| HD 36576 | 120 Tau | B2 | IV-V | 266 ± 13 | 22618 ± 508 | 3.804 ± 0.062 |
| HD 37490 | ω Ori | B3 | V | 155 ± 5(e) | 14 492(h) | 3.86(h) |
| HD 41335 | V696 Mon | B3-5 | V | 376 ± 26 | 20902 ± 610 | 3.886 ± 0.081 |
| HD 68980 | MX Pup | B1.5 | IV | 152±8 | 25 126 ± 642 | 3.951 ± 0.077 |
| HD 142983 | 48 Lib | B3 (f) | V(f) | 407 ± 22 | 17 642 ± 554 | 3.845 ± 0.080 |
| HD 155806 | V1075 Sco | O7.5 | V | 105 ± 16(c) | 34000(i) | 4.0(i) |
| HD 164284 | 66 Oph | B2 | V | 287 ± 21 | 21 609 ± 523 | 3.943 ± 0.068 |
| HD 171623 | HR 6977 | A0 | V | 253 ± 38(c) | 9853 ± 291(j) | 3.91 ± 0.23(j) |
| HD 178175 | V4024 Sgr | B2 | V | 111 ± 7 | 18 939 ± 286 | 3.489 ± 0.035 |
| HD 183656 | V923 Aql | B7 | III | 284 ± 16 | 12 626 ± 524 | 3.295 ± 0.081 |
| HD 187811 | 12 Vul | B2.5 | V | 258 ± 13 | 18 086 ± 583 | 3.810 ± 0.083 |
| HD 191610 | 28 Cyg | B2.5 | V | 318 ± 22 | 18 353 ± 516 | 3.718 ± 0.072 |
| HD 209409 | o Aqr | B7 | IV | 282 ± 20 | 12 942 ± 402 | 3.701 ± 0.067 |
| HD 212571 | π Aqr | B1 | III-IV | 233 ± 15 | 26 061 ± 736 | 3.915 ± 0.088 |
| HD 217050 | EW Lac | B4 | III | 355 ± 25 | 17 893 ± 509 | 3.571 ± 0.070 |
Notes. (a) CDS database, except other source is indicated; (b) Frémat et al. (2005), except other source is indicated; (c) Głebocki & Gnaciński (2005); (d) Abt et al. (2002); (e) Chauville et al. (2001); (f) Zorec et al. (2005). (g) Using Teff and log g from other stars with the same ST; (h) Cochetti et al. (2019); (i) Cox & Pilachowski (2000);(j) Cochetti et al. (2020).
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