1996PASP..108..672C

Query : 1996PASP..108..672C

1996PASP..108..672C - Publ. Astron. Soc. Pac., 108, 672-681 (1996/August-0)

DDO metal abundances of high-luminosity late-type stars in galactic open clusters.

CLARIA J.J., PIATTI A.E. and OSBORN W.

Abstract (from CDS):

Result. from UBV and DDO photometry are presented for 54 high-luminosity late-type stars in the fields of 23 open clusters. The probability of cluster membership for each observed star is evaluated using two independent photometric criteria. It is found that 32 stars are very likely cluster members, the remaining ones being almost ceterainly field objects. The recently improved calibrations of the DDO system have been used to derive MK spectral types, effective temperatures, and metallicities, while E(B-V) color excesses have been determined through known photometric and spectroscopic procedures. The DDO metallicities range between values typical of moderately metal-poor ([Fe/H]≃ -0.3) to moderately metal-rich ([Fe/H] ≃ 0.2) clusters. The masses of the cluster giants range between 1 and 4 solar masses, with the scatter within a cluster being less than 1 solar mass.

Abstract Copyright: ∼

Journal keyword(s): Stellar Clusters and Associations

CDS comments: table 3 : CL Stock 2 82a not in SIMBAD

Simbad objects: 81

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Number of rows : 81
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* DL Cas cC* 00 29 58.5888773064 +60 12 43.065292140 10.66 9.88 8.63   7.582 G1Ib-IIHdel-1 349 0
2 HD 236433 SB* 00 30 06.0055796736 +60 09 04.103352540 10.50 9.83 8.87     F4II 60 0
3 NGC 129 OpC 00 30 25.8 +60 12 44   7.33 6.5     ~ 216 0
4 HD 236446 * 00 31 25.4682391272 +60 15 19.605628332 12.63 10.55 8.71     M0IIp 28 0
5 HD 236449 * 00 31 38.3348049240 +60 15 19.394164188 12.64 10.56 8.57     K2.5II-III 25 0
6 NGC 225 OpC 00 42 34.7 +61 47 30   7.43 7.0     ~ 110 0
7 BD+60 86 * 00 43 18.2269462992 +61 45 37.436128488   11.22 9.69     K2III 10 0
8 BD+60 91 * 00 43 52.0696263864 +61 44 18.206418876   10.73 9.85     G6III 21 0
9 M 103 OpC 01 33 21.1 +60 39 13   7.72 7.4     ~ 212 0
10 BD+59 274 V* 01 33 29.2148328144 +60 38 47.710826664 12.90 10.64 8.54     M0.5Ib-II 51 0
11 BD+37 407 * 01 55 12.6246242616 +37 50 14.552504052   10.31 9.39     G5III 73 0
12 BD+37 418 SB* 01 56 18.8975265744 +37 58 00.460205436   9.98 8.97     G9III 36 0
13 BD+36 358 * 01 56 21.6380682480 +37 36 08.432374752   10.54 9.43     K0III 68 0
14 HD 11811 MS* 01 56 50.4332970624 +38 01 58.141549236   9.75 8.91     G2V 44 0
15 NGC 752 OpC 01 56 53.7 +37 45 06           ~ 712 0
16 BD+37 428 * 01 57 25.9123941744 +37 51 42.695591832   11.13 10.19     G8III 22 0
17 BD+36 368 SB* 01 57 37.5961724736 +37 39 37.908040644   9.90 8.85     K1III 44 1
18 BD+37 432 * 01 57 38.9498019528 +37 46 12.414071532   9.98 9.00     G9III 70 0
19 BD+37 441 Em* 01 58 29.8173119448 +37 51 37.575588024   10.23 9.29     G5 79 0
20 BD+37 448 * 01 58 52.9027843464 +37 48 57.229263828   10.07 9.04     K0III 93 0
21 HD 13209 * 02 10 38.7022812912 +53 12 53.088502896   8.22 8.17     A0 21 0
22 HD 13437 * 02 13 28.7858368200 +59 11 45.593710080   8.78 7.61     G5II 52 0
23 Cl Stock 2 OpC 02 15 47.8 +59 33 12           ~ 155 0
24 BD+58 424 SB* 02 16 20.1265114296 +59 20 19.005339912   10.33 9.24     G8III 9 0
25 HD 14173 * 02 19 41.5271206848 +60 00 46.994528196   8.16 7.19     G5II 37 0
26 Cl Trumpler 2 OpC 02 36 14.9 +55 54 32           ~ 124 0
27 HD 16068 * 02 36 52.7997095160 +55 54 55.443018600   9.18 7.45     K3II-III 40 0
28 NGC 1027 OpC 02 42 38.2 +61 36 49   7.28 6.7     ~ 109 0
29 BD+60 551 SB* 02 42 56.1483344568 +61 36 47.762623548   10.93 9.51     ~ 8 0
30 HD 25497 * 04 06 39.3850519056 +62 20 04.700879340   9.89 9.62     A3V:n 17 0
31 HD 25498 SB* 04 06 43.0797405888 +62 20 40.291900836   9.12 7.93     K 23 0
32 NGC 1502 OpC 04 07 49.4 +62 19 35   7.47 6.9     ~ 202 1
33 NGC 1545 OpC 04 20 53.3 +50 11 32   7.2 6.2     ~ 121 0
34 HD 27277 * 04 20 53.5488625632 +50 16 18.210679032   9.05 8.11     G6III 27 0
35 HD 27292 * 04 20 57.5014421472 +50 15 17.412424956   8.77 7.13     K2+III 40 0
36 HD 30485 * 04 48 29.5100023824 +10 55 48.267667596   9.52 8.34     G8III 37 0
37 HD 287148 * 04 48 32.0830639248 +10 57 59.017301856   10.03 8.87     G5 41 0
38 NGC 1662 OpC 04 48 48.5 +10 52 46   7.0 6.4     ~ 149 0
39 HD 276826 * 04 49 05.6010911760 +43 36 48.721124088   10.7 8.90     K5 12 0
40 HD 30410 SB* 04 49 25.9879375368 +43 32 32.111604240   8.47 7.53     G8V 16 0
41 NGC 1664 OpC 04 50 59.3 +43 39 48           ~ 143 0
42 Cl Trumpler 9 OpC 07 55 39.8 -25 53 20   8.96 8.7     ~ 53 0
43 CD-25 5282 PM* 07 55 46.0748822400 -25 53 44.955246300   10.82 10.09     ~ 5 0
44 NGC 2489 36 * 07 56 09.4413796488 -30 03 29.088862776   13.404 12.112     K: 8 0
45 CD-29 5178 * 07 56 09.9714120432 -30 02 54.417735060   12.44 10.97     ~ 12 0
46 NGC 2489 14 * 07 56 14.7800102088 -30 02 48.923519172   13.101 11.752     ~ 5 0
47 NGC 2489 OpC 07 56 15.7 -30 03 35   8.58 7.9     ~ 83 0
48 CD-29 5182 * 07 56 17.1791815368 -30 03 41.765956524   12.63 11.49     ~ 7 0
49 NGC 2489 50 * 07 56 19.6862679424 -30 05 31.914618774   13.027 11.765     ~ 6 0
50 NGC 2489 25 SB* 07 56 20.1149518272 -30 05 00.085754220   13.273 11.937     ~ 9 0
51 * 35 Cnc RG* 08 35 19.4461296744 +19 35 24.230563692   7.248 6.558     G0III 150 0
52 HD 73598 ** 08 39 50.7154795152 +19 32 26.919638988   7.53 6.60     G8III-IIIb 130 0
53 NGC 2632 OpC 08 39 58.4 +19 36 33           ~ 1733 0
54 * 39 Cnc * 08 40 06.4182853944 +20 00 28.034963316 8.20 7.37 6.39 5.67 5.20 G8+III-IIIb 220 0
55 HD 73710 * 08 40 22.0864518288 +19 40 11.771283936 8.290 7.410 6.390 5.70 5.21 G9III-IIIb 201 0
56 HD 73974 SB* 08 41 50.0792800992 +19 52 27.045440112   7.88 6.92     G8III-IIIb 121 0
57 HD 91850 * 10 34 55.9659580968 -58 11 12.228668880 8.57 9.28 9.09 9.62   B0/1(III) 52 0
58 NGC 3293 OpC 10 35 50.3 -58 14 04           ~ 327 0
59 Cl Ruprecht 97 14 * 11 57 27.2220016320 -62 42 06.179262120   13.76 12.38     ~ 13 0
60 Cl Ruprecht 97 OpC 11 57 27.5 -62 42 26   9.77 9.1     ~ 47 0
61 Cl Ruprecht 97 21 * 11 57 36.6069950808 -62 43 52.433390460   14.12 12.36     ~ 4 0
62 Cl Ruprecht 97 4 * 11 57 48.8737755000 -62 37 43.747278852   13.64 12.39     ~ 6 0
63 Cl Ruprecht 97 3 * 11 57 51.1678988688 -62 37 08.468897736   13.31 12.11     ~ 6 0
64 Cl Ruprecht 98 8 * 11 59 04.5466128816 -64 33 20.231742240 14.01 12.09 10.34     K8/M0 6 0
65 Cl Ruprecht 98 OpC 11 59 32.8 -64 31 32           ~ 65 0
66 NGC 4463 OpC 12 29 54.0 -64 48 14   7.62 7.2     ~ 70 0
67 CPD-64 1943 * 12 29 55.3453659432 -64 48 40.774507092   9.05 8.33     F5Iab 26 0
68 NGC 6242 OpC 16 55 31.8 -39 28 09           ~ 98 0
69 HD 152524 * 16 55 37.8128350032 -39 30 17.916882012   9.09 7.28     K2II/III 26 0
70 Cl Collinder 399 Cl* 19 25.4 +20 11   3.93 3.6     ~ 21 0
71 HD 182955 * 19 26 28.6865078856 +19 53 29.381827056 9.29 7.39 5.87 4.69 3.65 M0III 63 0
72 BD+37 3862 * 20 16 32.4567217421 +37 38 42.224670180 8.93 9.09 8.78 9.09   B0IVp 36 0
73 IC 4996 OpC 20 16 32.7 +37 38 46           ~ 187 0
74 HD 228721 * 20 16 52.8482261520 +37 31 04.714995648   9.74 8.59     G9.5IIIb 16 0
75 NGC 7209 OpC 22 04 50.7 +46 30 11   8.24 7.7     ~ 144 0
76 BD+45 3792 * 22 05 17.6227942872 +46 29 00.629139984   10.80 9.45     K4 26 0
77 NGC 7209 105 * 22 05 41.9040288744 +46 33 07.493823072   11.76 11.63     B7 15 0
78 BD+45 3800 PM* 22 05 46.2724503936 +46 41 55.001384124   10.10 9.58     F8 7 0
79 BD+45 3801 s*r 22 05 59.2011087720 +46 27 17.388284256   10.79 8.98     K5Ib 12 0
80 BD+60 2532 * 23 24 15.8452342152 +61 35 17.546649504   9.345 8.292 7.84   F8Ib/II 59 0
81 M 52 OpC 23 24 47.2 +61 35 32           ~ 200 0

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