VDBH 106

(BH 106; vdBergh-Hagen 106; MWSC 1863)

0.24 UTI

0.0

C_N

0.07

C_dens

0.25

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.07 Very loose
C_C3 0.25 Low quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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VDBH 106 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Relatively close Moderate extinction Old

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for VDBH 106 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–	163.14	-54.247	0.368	-7.471	2.514	7.536
Hunt & Reffert	2023	163.349	-54.248	0.376	-7.485	2.51	–
Just et al.	2023	163.15	-54.261	–	–	–	–
Bica et al.	2019	163.186	-54.269	–	–	–	–
Kharchenko et al.	2016	163.15	-54.261	–	–	–	–
Dias et al.	2014	163.175	-54.233	–	-6.88	0.74	–
Kharchenko et al.	2013	163.158	-54.265	–	-8.33	4.66	–
Bukowiecki et al.	2011	163.167	-54.262	–	–	–	–
Dias et al.	2002	163.175	-54.233	–	-6.88	0.74	–

💡 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–	2.785	1.13	1.09	1841	–	865	–	–
Hunt & Reffert	2023	2.43	0.45	1.09	8110	–	–	–	–
Just et al.	2023	–	–	–	1841	–	865	–	–
Kharchenko et al.	2016	3.14	1.13	–	1841	–	–	–	–
Kharchenko et al.	2013	3.14	1.13	–	1841	–	–	–	–
Dias et al.	2002	1.88	1.26	–	100	–	–	–	–

Visualization

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