CBB 3

0.14 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.52

C_dup

N₅₀ (P>50% members) 19

Stellar density (N₅₀/rad) 5.9 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CBB 3 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 14 years.

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

Relatively close Moderate extinction Very young

Data

🔍 Search references for CBB 3 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	81.911	34.567	0.455	-0.114	-2.097	–
Camargo et al.	2012	81.93	34.543	–	–	–	–

💡 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–	2.7	1.98	–	2	–	–	–	–
Camargo et al.	2012	2.70	1.98	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Stock 8	48.0	81.96	34.43	0.46	0.08	-2.34	-59.37	0.91
CBB 5	4.0	82.05	34.45	0.46	0.14	-2.09	11.91	0.16

💡 Note: The % column shows the percentage of members that CBB 3 shares with each listed object.

Visualization

ℹ️