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

Full paper

View the references in ADS

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 - 2023	#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	324	0
2	HD 236433	SB*	00 30 06.0055796736	+60 09 04.103352540	10.50	9.83	8.87			F4II	57	0
3	NGC 129	OpC	00 30 25.7	+60 12 47		7.33	6.5			~	200	0
4	HD 236446	*	00 31 25.4682391272	+60 15 19.605628332	12.63	10.55	8.71			M0IIp	27	0
5	HD 236449	*	00 31 38.3348049240	+60 15 19.394164188	12.64	10.56	8.57			K2.5II-III	23	0
6	NGC 225	OpC	00 43 13.2	+61 46 26		7.43	7.0			~	99	0
7	BD+60 86	*	00 43 18.2269462992	+61 45 37.436128488		11.22	9.69			K2III	9	0
8	BD+60 91	*	00 43 52.0696263864	+61 44 18.206418876		10.73	9.85			G6III	19	0
9	M 103	OpC	01 33 21.4	+60 39 32		7.72	7.4			~	200	0
10	BD+59 274	V*	01 33 29.2148328144	+60 38 47.710826664	12.90	10.64	8.54			M0.5Ib-II	47	0
11	BD+37 407	*	01 55 12.6246242616	+37 50 14.552504052		10.31	9.39			G5III	58	0
12	BD+37 418	SB*	01 56 18.8975265744	+37 58 00.460205436		9.98	8.97			G9III	33	0
13	BD+36 358	*	01 56 21.6380682480	+37 36 08.432374752		10.54	9.43			K0III	52	0
14	HD 11811	MS*	01 56 50.4332970624	+38 01 58.141549236		9.75	8.91			G2V	38	0
15	NGC 752	OpC	01 56 53.5	+37 47 38						~	628	0
16	BD+37 428	*	01 57 25.9123941744	+37 51 42.695591832		11.13	10.19			G8III	21	0
17	BD+36 368	SB*	01 57 37.5961724736	+37 39 37.908040644		9.90	8.85			K1III	41	1
18	BD+37 432	*	01 57 38.9498019528	+37 46 12.414071532		9.98	9.00			G9III	60	0
19	BD+37 441	*	01 58 29.8173119448	+37 51 37.575588024		10.23	9.29			G8III	59	0
20	BD+37 448	*	01 58 52.9027843464	+37 48 57.229263828		10.07	9.04			G9III	81	0
21	HD 13209	*	02 10 38.7022812912	+53 12 53.088502896		8.22	8.17			A0	19	0
22	HD 13437	*	02 13 28.7858368200	+59 11 45.593710080		8.78	7.61			G5II	41	0
23	Cl Stock 2	OpC	02 15 25.4	+59 31 19						~	121	0
24	BD+58 424	SB*	02 16 20.1265114296	+59 20 19.005339912		10.33	9.24			G8III	7	0
25	HD 14173	*	02 19 41.5271206848	+60 00 46.994528196		8.16	7.19			G5II	33	0
26	HD 16068	*	02 36 52.7997095160	+55 54 55.443018600		9.18	7.45			K3II-III	33	0
27	Cl Trumpler 2	OpC	02 36 55.7	+55 54 18						~	109	0
28	NGC 1027	OpC	02 42 42.5	+61 36 58		7.28	6.7			~	90	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	16	0
31	HD 25498	SB*	04 06 43.0797405888	+62 20 40.291900836		9.12	7.93			K	20	0
32	NGC 1502	OpC	04 07 49.0	+62 19 55		7.47	6.9			~	189	1
33	NGC 1545	OpC	04 20 48.5	+50 13 16		7.2	6.2			~	107	0
34	HD 27277	*	04 20 53.5488625632	+50 16 18.210679032		9.05	8.11			G6III	25	0
35	HD 27292	*	04 20 57.5014421472	+50 15 17.412424956		8.77	7.13			K2+III	35	0
36	HD 30485	*	04 48 29.5100023824	+10 55 48.267667596		9.52	8.34			G8III	28	0
37	HD 287148	*	04 48 32.0830639248	+10 57 59.017301856		10.03	8.87			G5	32	0
38	NGC 1662	OpC	04 48 47.5	+10 52 55		7.0	6.4			~	131	0
39	HD 276826	*	04 49 05.6010911760	+43 36 48.721124088		10.7	8.90			K5	10	0
40	HD 30410	*	04 49 25.9879375368	+43 32 32.111604240		8.47	7.53			G8V	13	0
41	NGC 1664	OpC	04 51 03.1	+43 40 34		8.02	7.6			~	124	0
42	Cl Trumpler 9	OpC	07 55 39	-25 53.3		8.96	8.7			~	47	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			~	11	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 15.4	-30 03 36		8.58	7.9			~	76	0
48	CD-29 5182	*	07 56 17.1791815368	-30 03 41.765956524		12.63	11.49			~	6	0
49	NGC 2489 50	*	07 56 19.6862251329	-30 05 31.914006225		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	*	08 35 19.4461296744	+19 35 24.230563692		7.248	6.558			G0III	136	0
52	HD 73598	**	08 39 50.7154795152	+19 32 26.919638988		7.53	6.60			G8III-IIIb	118	0
53	* 39 Cnc	*	08 40 06.4182853944	+20 00 28.034963316	8.20	7.37	6.39	5.67	5.20	G8+III-IIIb	192	0
54	NGC 2632	OpC	08 40 13.0	+19 37 16						~	1509	0
55	HD 73710	*	08 40 22.0864518288	+19 40 11.771283936	8.290	7.410	6.390	5.70	5.21	G9III-IIIb	178	0
56	HD 73974	SB*	08 41 50.0792800992	+19 52 27.045440112		7.88	6.92			G8III-IIIb	110	0
57	HD 91850	*	10 34 55.9659580968	-58 11 12.228668880	8.57	9.28	9.09	9.62		B0/1(III)	47	0
58	NGC 3293	OpC	10 35 52.8	-58 13 52						~	309	0
59	Cl Ruprecht 97 14	*	11 57 27.2220016320	-62 42 06.179262120		13.76	12.38			~	10	0
60	Cl Ruprecht 97	OpC	11 57 28.6	-62 42 29		9.77	9.1			~	42	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	OpC	11 58 51.6	-64 34 52						~	51	0
65	Cl Ruprecht 98 8	*	11 59 04.5466128816	-64 33 20.231742240	14.01	12.09	10.34			K8/M0	5	0
66	NGC 4463	OpC	12 29 51.8	-64 48 00		7.62	7.2			~	64	0
67	CPD-64 1943	*	12 29 55.3453659432	-64 48 40.774507092		9.05	8.33			F5Iab	25	0
68	NGC 6242	OpC	16 55 30.7	-39 28 26						~	86	0
69	HD 152524	*	16 55 37.8128350032	-39 30 17.916882012		9.09	7.28			K2II/III	23	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	61	0
72	IC 4996	OpC	20 16 32.4	+37 38 56						~	175	0
73	BD+37 3862	*	20 16 32.4567217421	+37 38 42.224670180	8.93	9.09	8.78	9.09		B0IVp	34	0
74	HD 228721	*	20 16 52.8482261520	+37 31 04.714995648		9.74	8.59			G9.5IIIb	14	0
75	NGC 7209	OpC	22 04 53.8	+46 30 29		8.24	7.7			~	125	0
76	BD+45 3792	*	22 05 17.6227942872	+46 29 00.629139984		10.80	9.45			K4	23	0
77	NGC 7209 105	*	22 05 41.9040288744	+46 33 07.493823072		11.76	11.63			B7	12	0
78	BD+45 3800	PM*	22 05 46.2724503936	+46 41 55.001384124		10.10	9.58			F8	6	0
79	BD+45 3801	s*r	22 05 59.2011087720	+46 27 17.388284256		10.79	8.98			K5Ib	10	0
80	BD+60 2532	*	23 24 15.8452342152	+61 35 17.546649504		9.345	8.292	7.84		F8Ib/II	55	0
81	M 52	OpC	23 24 46.8	+61 35 24						~	189	0

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