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Table 4.

Data of the selected sample of Cepheids.

Cepheid RA
h:m:s (J2000)		 Dec
d:m:s (J2000)		 Galactocentrica
distance (kpc)		 Massb
M⊙		 [C/H]c
dex		 [N/H]c
dex		 [O/H]c
dex		 [Na/H]d
dex		 [Fe/H]d
dex
AQ Pup 07:58:22.09 −29:07:48.34 9.472±0.436 9.14±0.53 −0.44 0.25 −0.14 0.36±0.00 0.06±0.05
BB Sgr 18:50:59.87 −20:17:42.83 7.203±0.452 4.97±0.23 – – – 0.49 0.11
BF Oph 17:06:05.50 −26:34:50.03 7.081±0.452 3.42±0.17 −0.13 0.44 0.21 0.41 0.13
BN Pup 08:06:21.48 −30:05:48.77 9.930±0.428 6.44±0.40 −0.31 0.53 0.24 0.22±0.02 0.03±0.05
CV Mon 06:37:04.85 +03:03:50.28 9.362±0.452 4.08±0.21 −0.30 0.20 0.05 0.31±0.20 0.09±0.09
δ Cep 22:29:10.27 +58:24:54.71 8.010±0.452 4.53±0.26 −0.17 0.36 0.23 0.38 0.11
η Aql 19:52:28.37 +01:00:20.37 7.750±0.452 4.36±0.25 – – – 0.33 0.11
EV Sct 18:36:39.60 −08:11:05.36 – 5.46±0.60 −0.23 0.32 0.23 0.25±0.00 0.09±0.07
KN Cen 13:36:36.90 −64:33:29.92 – 12.45±0.72 −0.04 0.42 0.33 0.69±0.04 0.55±0.12
l Car 09:45:14.81 −62:30:28.45 7.845±0.451 13.71±0.66 −0.11 0.04 0.22 0.09 0.17
RS Pup 08:13:04.22 −34:34:42.70 8.585±0.444 12.79±0.94 −0.54 0.54 0.56 0.75 0.14
RY Sco 17:50:52.34 −33:42:20.42 6.663±0.453 6.22±0.32 – – – 0.36±0.06 0.01±0.06
RY Vel 10:20:41.03 −55:19:17.03 7.774±0.432 8.51±0.41 −0.05 0.40 0.29 0.46 0.02
RZ Vel 08:37:01.30 −44:06:52.85 8.249±0.445 7.89±0.38 −0.33 0.18 0.09 0.45 0.12
S Nor 16:18:51.83 −57:53:59.25 7.232±0.451 6.64±0.32 −0.12 0.38 0.21 0.45 0.06
SU Cas 02:51:58.75 +68:53:18.60 8.229±0.451 6.56±0.51 – – – 0.39 0.09
SV Vul 19:51:30.91 +27:27:36.84 7.284±0.438 13.93±0.74 – – – 0.18 0.08
SW Vel 08:43:38.69 −47:24:11.20 8.457±0.433 7.35±0.34 −0.46 0.49 0.04 0.23 −0.07
T Mon 06:25:13.00 +07:05:08.56 9.056±0.452 10.23±0.68 −0.15 0.47 0.33 0.53 0.00
T Vel 08:37:40.82 −47:21:43.08 8.084±0.448 3.30±0.23 −0.35 0.17 0.07 0.35 0.05
U Car 10:57:48.19 −59:43:55.88 7.574±0.443 8.15±0.39 0.17 0.42 0.07 0.53 0.21
U Nor 15:42:20.92 −55:18:42.94 6.876±0.450 5.90±0.41 0.09 0.56 0.40 0.41 0.11
U Sgr 18:31:53.33 −19:07:30.26 7.371±0.452 4.50±0.20 – – – 0.34 0.11
UU Mus 11:52:17.73 −65:24:15.06 7.097±0.414 6.00±0.54 −0.22 0.37 0.12 0.37 0.15
V340 Nor 16:13:17.68 −54:14:05.06 – 5.09±0.23 −0.08 0.34 0.27 0.40±0.00 0.07±0.07
V Cen 14:32:33.08 −56:53:15.78 7.459±0.451 4.35±0.31 −0.22 0.30 0.11 0.38 0.08
VW Cen 13:33:59.03 −64:03:20.00 – 6.11±0.32 – – – 0.79±0.05 0.41±0.08
VY Car 10:44:32.70 −57:33:55.33 7.627±0.441 8.47±0.39 −0.21 0.59 0.17 0.31 0.01
WZ Car 10:55:18.73 −60:56:23.95 7.601±0.396 6.47±0.49 −0.40 0.11 −0.09 0.53 0.02
WZ Sgr 18:16:59.72 −19:04:32.97 6.326±0.453 8.22±0.49 – – – 0.59±0.07 0.28±0.08
X Cyg 20:43:24.19 +35:35:16.07 7.772±0.448 8.61±0.40 – – – 0.38 0.13
XX Cen 20:43:24.19 +35:35:16.07 7.015±0.445 5.69±0.26 −0.17 0.39 0.19 0.34 0.06

Notes.

(a)

Distances from Genovali et al. (2014). The distances were computed from near-IR period-Wesenheit relations (Inno et al. 2013).

(b)

Pulsation masses of Milky Way Cepheids derived using predicted period-luminosity-colour relations with Z = 0.02 and Y = 0.25–0.31 (Caputo et al. 2005).

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