OC 0217

0.00 UTI

0.5

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 51

Radius (P>50% members) 2.0 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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OC 0217 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for OC 0217 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	2.531	61.184	0.248	-2.717	-0.883	-59.686
Hao et al.	2022	2.499	61.172	0.255	-2.704	-0.883	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Hao et al.	2022	–	2.90	–	316	0.112	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
King 13	100.0	2.55	61.17	0.25	-2.73	-0.87	-59.85	1.0
OC 0216	43.1	2.51	61.17	0.25	-2.75	-0.88	-59.69	0.0
OC 0215	39.2	2.51	61.17	0.23	-2.72	-0.87	-59.66	0.0
OC 0218	15.7	2.51	61.15	0.26	-2.74	-0.83	-58.07	0.0
OC 0219	15.7	2.64	61.19	0.26	-2.73	-0.84	-61.3	0.0

💡 Note: The % column shows the percentage of members that OC 0217 shares with each listed object.

Visualization

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