OC 0180

0.27 UTI

0.41

C_N

0.21

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 41

Core radius and density 2.5 [pc], 1.1 [pc^-2]

C3 classification AB

C_N 0.41 Poorly populated
C_dens 0.21 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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OC 0180 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

High extinction Near-solar metallicity Very young

Data

🔍 Search references for OC 0180 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	99999–	331.192	62.279	1.07	-1.486	-2.716	-15.552
Hao et al.	2022	331.277	62.24	1.067	-1.537	-2.745	20.16

💡 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]	B_frac	BSS
UCC	99999–	–	3.07	–	5	0.265	–	–	–
Hao et al.	2022	–	3.07	–	5	0.265	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1038	100.0	330.64	62.33	1.08	-1.48	-2.72	-20.98	0.27

💡 Note: The % column shows the percentage of members that OC 0180 shares with each listed object.

Visualization

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