OC 0214

0.17 UTI

0.0

C_N

0.6

C_dens

0.75

C_C3

0.0

C_lit

0.64

C_dup

C3 classification AB

Number of members (P>50%) 23

Radius (P>50% members) 3.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.6 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

ℹ️

OC 0214 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Low extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0214 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	0.775	60.993	0.315	-3.042	-1.488	–
Hao et al.	2022	0.807	60.991	0.32	-3.01	-1.512	–

💡 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	–	0.74	–	16	0.414	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 406	36.0	0.58	60.97	0.27	-3.14	-1.51	–	0.44

💡 Note: The % column shows the percentage of members that OC 0214 shares with each listed object.

Visualization

ℹ️