VDBH 174

(Lynga 4; MWSC 2302; OCL 941; vdBergh-Hagen 174; ESO 147 07)

0.84 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.84

C_lit

1.0

C_dup

N₅₀ (P>50% members) 101

Stellar density (N₅₀/rad) 33.8 [N/pc²]

C3 classification AB

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.84 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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VDBH 174 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.

Relatively close High extinction Near-solar metallicity Intermediate age

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Cavallo et al. (2024)
Gold sample.

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Data

🔍 Search references for VDBH 174 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–	233.333	-55.232	0.387	-4.011	-3.052	-27.429
Almeida et al.	2025	233.342	-55.24	–	–	–	–
Hunt & Reffert	2024	233.333	-55.235	0.395	-4.016	-3.047	-0.231
Cavallo et al.	2024	233.342	-55.24	0.394	–	–	–
Hunt & Reffert	2023	233.333	-55.235	0.395	-4.016	-3.047	-0.231
Just et al.	2023	233.321	-55.239	–	–	–	–
Dias et al.	2021	233.342	-55.24	0.345	-4.038	-2.984	-47.459
Cantat-Gaudin et al.	2020	233.344	-55.234	0.35	-3.983	-3.004	–
Cantat-Gaudin & Anders	2020	233.344	-55.234	0.35	-3.983	-3.004	–
Soubiran et al.	2018	233.344	-55.234	–	–	–	-46.08
Bica et al.	2019	233.33	-55.244	–	–	–	–
Cantat-Gaudin et al.	2018	233.344	-55.234	0.35	-3.983	-3.004	–
Kharchenko et al.	2016	233.321	-55.239	–	–	–	–
Dias et al.	2014	233.329	-55.236	–	-3.01	-1.88	–
Kharchenko et al.	2013	233.332	-55.24	–	-7.0	-3.69	–
Morales et al.	2013	233.329	-55.236	–	–	–	–
Bukowiecki et al.	2011	233.346	-55.208	–	–	–	–
Dias et al.	2002	233.329	-55.236	–	-3.01	-1.88	–

💡 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–	2.11	3.97	2.85	355	0.302	640	–	–
Almeida et al.	2025	2.11	3.91	–	39	–	640	–	–
Hunt & Reffert	2024	–	–	–	–	–	1694⁽¹⁾	–	–
Cavallo et al.	2024	2.28	4.82	–	95	0.420	–	–	–
Hunt & Reffert	2023	2.30	5.06	2.85	104	–	–	–	–
Just et al.	2023	–	–	–	355	–	96	–	–
Dias et al.	2021	2.11	3.91	–	39	0.185	–	–	–
Cantat-Gaudin & Anders	2020	2.64	–	–	–	–	–	–	–
Soubiran et al.	2018	2.64	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.64	–	–	–	–	–	–	–
Kharchenko et al.	2016	1.37	4.03	–	355	–	–	–	–
Kharchenko et al.	2013	1.37	4.03	–	355	–	–	–	–
Morales et al.	2013	1.10	–	–	1300	–	–	–	–
Bukowiecki et al.	2011	1.64⁽¹⁾	1.98	–	1995	–	–	–	–
Dias et al.	2002	1.10	2.17	–	1288	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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