VDBH 211

(BH 211; vdBergh-Hagen 211; MWSC 2518; ESO 332 16)

0.91 UTI

0.79

C_N

1.0

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 209

Stellar density (N₅₀/rad) 24.1 [N/pc²]

C3 classification AB

C_N 0.79 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 1.0 Very 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 211 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Palma et al. (2025)
Classified as optical pair P272, along with BH_202.

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: intermediate fit. Isochrone match: intermediate fit.

Data

🔍 Search references for VDBH 211 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–	255.522	-41.121	0.553	-0.695	-1.947	-48.342
Hu & Soubiran	2025	255.518	-41.124	–	–	–	–
Almeida et al.	2025	255.541	-41.124	–	–	–	–
Hunt & Reffert	2024	255.527	-41.112	0.572	-0.71	-1.923	-53.127
Cavallo et al.	2024	255.518	-41.124	0.57	–	–	–
Hunt & Reffert	2023	255.527	-41.112	0.572	-0.71	-1.923	-53.127
Just et al.	2023	255.535	-41.11	–	–	–	–
Dias et al.	2021	255.541	-41.124	0.51	-0.669	-1.951	-48.896
Spina et al.	2021	255.53	-41.12	0.507	-0.689	-1.939	–
Cantat-Gaudin et al.	2020	255.535	-41.113	0.524	-0.671	-1.943	–
Sánchez et al.	2020	255.546	-41.1	–	-0.726	-1.875	–
Donor et al.	2020	255.546	-41.1	–	-0.68	-2.04	-49.0
Cantat-Gaudin & Anders	2020	255.535	-41.113	0.524	-0.671	-1.943	–
Soubiran et al.	2018	255.535	-41.113	–	–	–	-48.83
Bica et al.	2019	255.549	-41.109	–	–	–	–
Cantat-Gaudin et al.	2018	255.535	-41.113	0.524	-0.671	-1.943	–
Kharchenko et al.	2016	255.535	-41.11	–	–	–	–
Dias et al.	2014	255.546	-41.1	–	-2.32	-2.67	–
Kharchenko et al.	2013	255.546	-41.11	–	-1.48	-2.29	–
Morales et al.	2013	255.546	-41.1	–	–	–	–
Bukowiecki et al.	2011	255.537	-41.083	–	–	–	–
Dias et al.	2002	255.546	-41.1	–	-3.45	-3.13	–

💡 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–	1.74	2.39	2.04	548	0.124	367	–	–
Hu & Soubiran	2025	–	–	–	–	-0.220⁽⁵⁾	–	–	–
Almeida et al.	2025	1.64	2.39	–	668	–	558	–	–
Hunt & Reffert	2024	–	–	–	–	–	1078⁽¹⁾	–	–
Cavallo et al.	2024	1.39	2.85	–	676	-0.250	–	–	–
Hunt & Reffert	2023	1.65	2.63	2.04	171	–	–	–	–
Just et al.	2023	–	–	–	331	–	126	–	–
Dias et al.	2021	1.64	2.39	–	668	0.124	–	–	–
Spina et al.	2021	2.01	–	–	427	0.214⁽²⁰⁾	–	–	–
Cantat-Gaudin et al.	2020	1.91	2.18	–	427	–	–	–	–
Donor et al.	2020	–	–	–	–	0.210	–	–	–
Cantat-Gaudin & Anders	2020	1.81	–	–	–	–	–	–	–
Soubiran et al.	2018	1.81	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.81	–	–	–	–	–	–	–
Kharchenko et al.	2016	1.82	3.32	–	331	–	–	–	–
Kharchenko et al.	2013	1.82	3.32	–	331	–	–	–	–
Morales et al.	2013	1.38	–	–	1585	–	–	–	–
Bukowiecki et al.	2012	–	–	–	–	–	176	–	–
Bukowiecki et al.	2011	1.67⁽¹⁾	1.46	–	1585	–	–	–	–
Dias et al.	2002	1.44	1.89	–	1000	–	–	–	–

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

Visualization

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