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Table 11

NGC 3114: Stellar fundamental parameters from the BCD system.

ID Other D λ1 Φb S.T Teff log g Mv Mbol
Lynga designation [dex] [Å] [μ] [K] [dex] [mag] [mag] [μ]
003 HD 87 458 dd 0.27 39 0.42 B6IIIe 15 349 ± 920 3.18 ± 0.28 −1.90 ± 0.57 −2.83 ± 0.60 0.78 ± 0.01
004 HD 87 241 dd 0.38 37 1.13 B8IIIp,e 12 250 ± 506 3.10 ± 0.28 −0.99 ± 0.41 −1.89 ± 0.57 0.85 ± 0.02
005 HD 87 266 0.18 47 0.62 B2IIIp 20 521 ± 1161 3.61 ± 0.34 −2.51 ± 0.55 −4.04 ± 0.43 0.72 ± 0.01
006 HD 87 137 dd 0.38 53 0.73 B8IV 11 886 ± 277 4.02 ± 0.21 −0.04 ± 0.30 −0.86 ± 0.26 0.85 ± 0.02
007 HD 87 042 0.46 100 0.78 A0Vmk 9790 ± 500a 4.14 ± 0.30a 0.65 ± 0.50a 0.35 ± 0.50a 1.07 ± 0.02m
009 HD 87 222 0.19 47 0.71 B3IVp 20 203 ± 1245 3.63 ± 0.32 −2.39 ± 0.53 −3.87 ± 0.44 0.72 ± 0.01
010 HD 87 349 0.34 50 0.22 B7V 13 079 ± 469 3.91 ± 0.23 −0.39 ± 0.32 −1.16 ± 0.34 0.81 ± 0.01
011 HD 87 031 dd 0.37 52 0.87 B8IV 12 341 ± 296 4.01 ± 0.21 −0.17 ± 0.31 −0.94 ± 0.25 0.84 ± 0.02
013 HD 304 848 0.34 53 0.77 B7V 12 906 ± 533 4.03 ± 0.20 −0.28 ± 0.27 −1.09 ± 0.27 0.81 ± 0.01
015 HD 87 612 0.24 52 0.66 B4V 16 908 ± 630 3.98 ± 0.23 −1.31 ± 0.35 −2.54 ± 0.41 0.75 ± 0.01
028 HD 87 404 dd 0.31 43 0.70 B6IVBe 14 309 ± 690 3.60 ± 0.30 −1.12 ± 0.45 −1.91 ± 0.50 0.79 ± 0.01
033 HD 87 818 dd 0.28 49 0.79 B5IVBe 14 912 ± 445 3.87 ± 0.25 −0.90 ± 0.38 −1.95 ± 0.42 0.78 ± 0.01
040 HD 304 894 0.43 66 0.25 A0V 10 741 ± 337 4.32 ± 0.11: 0.63 ± 0.37: 0.12 ± 0.24: 0.95 ± 0.04
047 HD 87 565 dd 0.21 74 0.30 B4VI:Be 19 031 ± 866: 4.35 ± 0.05: −1.40 ± 0.13: −2.74 ± 0.28: 0.75 ± 0.01
066 HD 304 841 0.32 56 0.94 B7V 13 530 ± 539 4.13 ± 0.15 −0.28 ± 0.20 −1.24 ± 0.28 0.80 ± 0.01
067 HD 304 840 0.40 59 1.05 B9V 11 596 ± 288 4.19 ± 0.16 0.36 ± 0.27 −0.53 ± 0.24 0.88 ± 0.03
079 HD 304 829 dd 0.40 89 1.27 A1Vmk 9395 ± 500a 4.17 ± 0.20a 0.98 ± 0.5a 0.73 ± 0.5a 1.14 ± 0.02m
085 CPD-59 1748 0.48 73 0.34 A2V: 9727 ± 270 4.44 ± 0.10: 0.46 ± 0.44: 0.27 ± 0.13f 1.07 ± 0.05
088 HD 304 837 0.49 62 0.85 A1V 9625 ± 368 4.14 ± 0.15 1.29 ± 0.41: 0.65 ± 0.46: 1.02 ± 0.05
091 HD 87 125 dd 0.37 48 0.99 B8IVshell,Boo 12 269 ± 311 3.82 ± 0.27 −0.40 ± 0.35 −1.07 ± 0.37 0.84 ± 0.02
097 HD 87 205 0.37 60 0.79 B8V 12 037 ± 318 4.22 ± 0.15 0.25 ± 0.31 −0.63 ± 0.24 0.85 ± 0.02
099 CPD-59 1677 0.41 59 1.10 B9V 11 465 ± 272 4.19 ± 0.15 0.46 ± 0.29 −0.46 ± 0.25: 0.89 ± 0.03
100 HD 304 836 0.40 74 0.97 A0VI: 11 134 ± 318 4.56 ± 0.11: −0.37 ± 0.36: −0.87 ± 0.30f 0.94 ± 0.03
102 HD 304 835 0.40 60 1.36 B9V 11 638 ± 328 4.20 ± 0.15 0.39 ± 0.32 −0.45 ± 0.28: 0.88 ± 0.03
105 CPD-59 1666 0.48 74 1.08 A2V:Boo 9565 ± 320 4.45 ± 0.30: 0.36 ± 0.40: 0.20 ± 0.30f 1.07 ± 0.05
124 HD 304 854 0.34 59 0.98 B7V 12 677 ± 487 4.21 ± 0.15 −0.04 ± 0.26 −0.89 ± 0.19 0.82 ± 0.02
126 HD 87 309 dd 0.39 52 1.05 B9IV 11 920 ± 308 3.98 ± 0.22 −0.05 ± 0.33 −0.89 ± 0.28 0.86 ± 0.02
127 HD 304 855 0.40 55 1.05 B9V 11 538 ± 268 4.09 ± 0.18 0.21 ± 0.26 −0.61 ± 0.28 0.87 ± 0.02
129 HD 87 366 dd 0.35 55 0.68 B8VBe 12 406 ± 364 4.11 ± 0.17 −0.09 ± 0.24 −0.92 ± 0.24 0.83 ± 0.02
130 HD 304 856 0.47 82 1.38 A5V: 8180 ± 500a 4.29 ± 0.30a 1.95 ± 0.50a 1.80 ± 0.50a 1.20 ± 0.05
132 HD 304 831 dd 0.29 72 1.03 B7:VI: 14 308 ± 648 4.40 ± 0.06: −0.83 ± 0.19: −1.57 ± 0.19: 0.81 ± 0.02:
134 HD 87 567 0.34 73 0.96 B9:VI: 12 383 ± 442 4.45 ± 0.06: −0.67 ± 0.24: −0.84 ± 0.14: 0.87 ± 0.03:
136 HD 87 581 0.32 50 0.97 B7IV 13 629 ± 416 3.90 ± 0.24 −0.55 ± 0.35 −1.35 ± 0.36 0.80 ± 0.01
141 HD 304 832 0.16 62 0.85 B2V 22 033 ± 916 4.15 ± 0.12 −1.93 ± 0.30 −3.76 ± 0.33 0.71 ± 0.00
147 HD 304 858 0.42 58 1.01 B9V 11 215 ± 274 4.13 ± 0.15 0.46 ± 0.24 −0.44 ± 0.29: 0.90 ± 0.02
149 HD 87 507 0.41 47 0.91 B9IV 11 650 ± 231 3.80 ± 0.27 −0.29 ± 0.36 −0.99 ± 0.34 0.87 ± 0.02
186 HD 86 981 0.30 69 0.73 B7VI: 13 851 ± 543 4.37 ± 0.08: −0.70 ± 0.19 −1.31 ± 0.17 0.81 ± 0.02
··· HD 304 838 0.41 63 1.09 B9V 11 155 ± 301 4.27 ± 0.14 0.53 ± 0.44: 0.03 ± 0.30f 0.91 ± 0.03
··· HD 87 436 dd 0.53 50 1.30 A7III: 7550 ± 500bv 3.05 ± 0.30a −0.19 ± 0.50f −0.16 ± 0.50a 1.79 ± 0.02m
··· HD 87 801 0.16 52 0.67 B2IVBe 21 613 ± 1127 3.87 ± 0.28 −2.43 ± 0.46 −4.16 ± 0.47 0.71 ± 0.00
··· HD 304 839 0.31 56 0.97 B6V 13 853 ± 586 4.15 ± 0.14 −0.30 ± 0.24 −1.24 ± 0.27 0.80 ± 0.01
··· CPD-59 1691 0.37 46 0.86 B8IV 12 323 ± 297 3.78 ± 0.28 −0.53 ± 0.37 −1.23 ± 0.39 0.83 ± 0.02
··· J10015881-6001125 0.41 55 0.60 B9V 11 371 ± 277 4.05 ± 0.18 0.20 ± 0.29 −0.64 ± 0.29 0.88 ± 0.02

Notes. Nomenclature according to Lyngå (1962). The symbol : is used to indicate extrapolated values. g is the stellar surface gravity given in cm s-2.

(dd)

Stars with a double Balmer discontinuity.

(mk)

Spectral type determined with the MK method.

(Be)

Known Be stars.

(e,shell)

Reported by González & Lapasset (2001).

(p)

Reported as peculiar stars in the literature.

(Boo)

Star reported as λBoothis variable by Schneider & Weiss (1988).

(a)

Values interpolated from Cox (2000).

(bv)

Teff values from Boehm-Vitense (1982).

(f)

Mbol values estimated with the bolometric correction given by Flower (1996).

(m)

Values determined using the relation between Φb and (B − V) given by Moujtahid et al. (1998).

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