Table 2
Adopted astrophysical quantities for our stars and final best-fit parameters.
| HD | HR | Name | N | Cl. | vsini | M∗ | R∗ | Δvpeak | vc | veq | i | ρ0 | Rd/R∗ | rem |
| (km s-1) | (M⊙) | (R⊙) | (km s-1) | (km s-1) | (km s-1) | (°) | (g cm-3) | |||||||
|
|
||||||||||||||
| 6811 | 335 | φ And | 3 | 2 | 80 | 4.0 | 3.1 | – | 500 | 400 | 12 | 8.50 × 10-14 | 6.4 | 3, 5 |
| 10516 | 496 | φ Per | 1 | 2 | 240 | 17.0 | 10.0 | 180 | 570 | 450 | 22 | 4.20 × 10-12 | 4.3 | 3, 4, 5 |
| 11415 | 542 | ϵ Cas | 1 | abs | 40 | 6.5 | 4.2 | – | – | – | – | – | – | – |
| 37202 | 1910 | ζ Tau | 2 | 2 | 120 | 10.5 | 6.1 | 290 | – | – | – | – | – | 1, 2, 3, 4, 5 |
| 37490 | 1934 | ω Ori | 2 | 1 | 180 | 8.9 | 5.1 | 190 | 580 | 460 | 23 | 8.00 × 10-12 | 3.1 | 1, 2, 3, 4 |
| 41335 | 2142 | V696 Mon | 2 | 2 | 310 | 8.9 | 5.1 | – | – | – | – | – | – | 1, 2, 3 |
| 43285 | 2231 | – | 1 | abs | 230 | 6.0 | 4.0 | – | – | – | – | – | – | – |
| 44458 | 2284 | FR CMa | 1 | 2 | 180 | 18.0 | 10.5 | 150 | 570 | 460 | 23 | 3.00 × 10-12 | 5.0 | 3 |
| 45542 | 2343 | ν Gem | 1 | sh | 160 | 5.1 | 3.5 | 175 | – | – | – | – | – | 2, 3, 4 |
| 47054 | 2418 | – | 1 | 1 | 180 | 4.0 | 3.1 | 140 | 500 | 400 | 27 | 3.80 × 10-13 | 5.8 | 3 |
| 50658 | 2568 | ψ09 Aur | 1 | sh | 230 | 4.5 | 3.3 | 150 | 510 | 400 | 80 | 3.50 × 10-14 | 8.5 | 3, 5 |
| 50820 | 2577 | – | 1 | 2 | 150 | 7.4 | 4.6 | – | 550 | 440 | 20 | 7.20 × 10-14 | 13.8 | – |
| 52918 | 2648 | 19 Mon | 1 | abs | 240 | 17.0 | 10.0 | – | – | – | – | – | – | – |
| 53416 | – | – | 1 | 1 | 190 | 4.0 | 3.5 | 120 | 470 | 370 | 30 | 7.60 × 10-14 | 9.1 | – |
| 58050 | 2817 | – | 3 | 1 | 110 | 9.0 | 5.3 | – | – | – | – | – | – | 3, 5 |
| 58343 | 2825 | FW CMa | 1 | 2 | 50 | 7.5 | 4.7 | – | 550 | 440 | 6 | 1.10 × 10-13 | 13.7 | 2, 3, 4 |
| 58715 | 2845 | β CMi | 3 | 1 | 210 | 3.8 | 3.0 | 130 | 490 | 390 | 32 | 1.25 × 10-13 | 7.0 | 2, 3, 4, 5 |
| 60855 | 2921 | V378 Pup | 1 | 2 | 240 | 9.0 | 5.3 | 150 | – | – | – | – | – | 2, 3 |
| 61224 | 2932 | – | 2 | 1 | 200 | 4.0 | 3.1 | 150 | 500 | 400 | 30 | 3.50 × 10-13 | 6.2 | 3 |
| 65875 | 3135 | V695 Mon | 3 | 2 | 180 | 12.0 | 7.0 | – | – | – | – | – | – | 2, 3 |
| 71072 | – | – | 2 | abs | 100 | 6.5 | 4.5 | – | – | – | – | – | – | – |
| 91120 | 4123 | – | 9 | 1 | 250 | 3.0 | 2.5 | 180 | 480 | 380 | 41 | 1.15 × 10-13 | 6.8 | 2, 3 |
| 109387 | 4787 | κ Dra | 13 | 1 ↔ 2 | 170 | 7.0 | 4.5 | 140 | 540 | 430 | 23 | 4.00 × 10-12 | 5.1 | 3, 5 |
| 138749 | 5778 | θ CrB | 11 | abs | 310 | 6.0 | 4.0 | – | – | – | – | – | – | 5 |
| 142926 | 5938 | V839 Her | 10 | sh | 275 | 4.0 | 3.1 | 240 | 500 | 400 | 44 | 6.00 × 10-12 | 4.3 | 5 |
| 142983 | 5941 | 48 Lib | 13 | sh | 390 | 4.1 | 3.2 | – | – | – | – | – | – | 2, 3 |
| 143275 | 5953 | δ Sco | 4 | 2 | 165 | 18.0 | 10.5 | – | – | – | – | – | – | 6 |
| 162428 | – | – | 5 | 1 | 240 | 4.0 | 3.0 | 180 | 500 | 400 | 36 | 9.00 × 10-12 | 6.1 | 4 |
| 162732 | 6664 | ζ Her | 6 | sh | 40 | 3.8 | 3.0 | 260 | – | – | – | – | – | 3, 5 |
| 164284 | 6712 | 66 Oph | 6 | 1 | 240 | 10.5 | 6.1 | 150 | 570 | 460 | 32 | 8.80 × 10-14 | 9.3 | 2, 3 |
| 164447 | 6720 | V974 Her | 4 | 1 | 180 | 4.0 | 3.5 | 140 | 470 | 370 | 28 | 1.75 × 10-13 | 5.8 | 5 |
| 183362 | 7403 | V558 Lyr | 4 | 2 | 220 | 9.0 | 5.3 | – | – | – | – | – | – | 3 |
| 183656 | 7415 | V923 Aql | 5 | sh | 190 | 3.8 | 3.0 | 250 | – | – | – | – | – | 2, 3 |
| 183914 | 7418 | β Cyg B | 5 | 1 | 240 | 4.0 | 3.0 | 160 | 500 | 400 | 37 | 9.00 × 10-14 | 8.2 | 3, 4 |
| 187567 | 7554 | V1339 Aql | 4 | 1 → 2 | 200 | 13.0 | 7.7 | 140 | 570 | 450 | 26 | 3.00 × 10-13 | 7.3 | – |
| 189687 | 7647 | 25 Cyg | 6 | sh | 230 | 7.5 | 4.7 | 250 | 550 | 440 | 31 | 3.05 × 10-13 | 3.6 | 3, 4 |
| 191610 | 7708 | 28 Cyg | 4 | 1 | 250 | 9.0 | 5.3 | 270 | 570 | 455 | 33 | 2.60 × 10-13 | 3.9 | 3, 4 |
| 192044 | 7719 | 20 Vul | 3 | 1 | 240 | 4.5 | 3.3 | 150 | 510 | 410 | 38 | 1.10 × 10-13 | 10.1 | – |
| 193911 | 7789 | 25 Vul | 3 | 1 | 170 | 4.0 | 3.5 | 100 | 470 | 370 | 27 | 2.30 × 10-13 | 6.0 | 2, 3, 5 |
| 210129 | 8438 | 25 Peg | 8 | 1 | 130 | 6.0 | 4.0 | 70 | 530 | 430 | 19 | 1.50 × 10-12 | 5.6 | 1, 2, 3 |
| 212571 | 8539 | π Aqr | 3 | 1 | 220 | 13.0 | 7.7 | 280 | 570 | 450 | 41 | 6.00 × 10-13 | 3.9 | 1, 2, 3, 4 |
| 214168 | 8603 | 8 Lac B | 3 | 2 | 150 | 17.0 | 10.0 | – | – | – | – | – | – | – |
| 216057 | 8682 | – | 4 | abs | 260 | 6.0 | 4.0 | – | – | – | – | – | – | – |
| 216200 | 8690 | 14 Lac | 3 | sh | 195 | 13.0 | 7.7 | – | – | – | – | – | – | 5 |
| 217050 | 8731 | – | 1 | sh | 240 | 6.0 | 4.0 | – | – | – | – | – | – | 3, 4, 5 |
| 217543 | 8758 | V378 And | 2 | sh | 305 | 7.5 | 4.7 | – | – | – | – | – | – | – |
| 217675 | 8762 | o And | 2 | sh | 200 | 6.0 | 4.0 | – | – | – | – | – | – | 4, 5 |
| 217891 | 8773 | β Psc | 6 | 2 | 75 | 6.0 | 4.0 | – | 535 | 430 | 10 | 5.20 × 10-13 | 6.1 | 1, 2, 4, 5 |
Notes. For each star we report, the number of spectra collected, their classification (abs means absorption lines only), the projected equatorial rotational velocity as measured by us in our spectra, mass and radius as estimated from Drilling & Landolt (1999), peaks separation, critical velocity, equatorial velocity, inclination angle, base density at the stellar equator, and the estimated disk radius. In the last column we also reported the references of other similar catalogs in which spectra of the star have been published: 1) Hanuschik (1988); 2) Hanuschik et al. (1996); 3) Hanuschik (1996); 4) Slettebak et al. (1992); 5) Saad et al. (2006); 6) Silaj et al. (2010).
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