G333.6-0.2

0.03 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 13

Core radius and density 3.0 [pc], 0.2 [pc^-2]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low 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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G333.6-0.2 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.

Note: This object shares a significant percentage of members with 6 later reported entries. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

🔍 Search references for G333.6-0.2 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–	245.613	-50.112	0.358	-2.731	-4.01	-14.277
Bica et al.	2003	245.532	-50.101	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
BDB2003 G333.60-00.21	68.0	245.6	-50.12	0.35	-2.74	-4.01	-29.65	0.02
UBC 543	16.0	245.73	-50.18	0.39	-2.36	-4.12	-71.96	0.1
CWWDL 13867	8.0	245.73	-50.18	0.41	-2.41	-4.1	-72.39	0.04
FoF 273	8.0	245.72	-50.18	0.39	-2.35	-4.12	-72.39	0.67
CWWDL 1589	4.0	245.73	-50.17	0.39	-2.36	-4.12	-71.96	0.0
DBSB 165	4.0	245.43	-50.42	0.4	-2.77	-4.11	-33.85	0.05

💡 Note: The % column shows the percentage of members that G333.6-0.2 shares with each listed object.

Visualization

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