VDB 130

(vdBergh 130; MWSC 3300)

0.82 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.79

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 137

Radius (P>50% members) 5.3 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.79 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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VDB 130 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Bronze sample.

Data

🔍 Search references for VDB 130 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	–	304.512	39.356	0.571	-3.587	-5.154	-23.664
Almeida et al.	2025	304.462	39.34	–	–	–	–
Hunt & Reffert	2024	304.517	39.367	0.581	-3.548	-5.127	-8.7
Cavallo et al.	2024	304.588	39.368	0.578	–	–	–
He et al.	2023	304.555	39.385	0.579	-3.62	-5.078	-18.44
Hunt & Reffert	2023	304.517	39.367	0.581	-3.548	-5.127	-8.7
Almeida et al.	2023	304.492	39.33	–	–	–	–
Just et al.	2023	304.42	39.348	–	–	–	–
Dias et al.	2021	304.462	39.34	0.521	-3.609	-5.075	–
Sánchez et al.	2020	304.425	39.35	–	-3.971	-4.889	–
Loktin & Popova	2017	304.425	39.35	–	-1.002	-1.194	–
Kharchenko et al.	2016	304.42	39.348	–	–	–	–
Dias et al.	2014	304.425	39.35	–	-3.61	-4.58	–
Kharchenko et al.	2013	304.425	39.35	–	-2.22	-4.39	–
Dias et al.	2002	304.425	39.35	–	-3.61	-4.58	–

💡 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]	Bfr	BSS
Almeida et al.	2025	1.46	2.36	–	9	–	380	–	–
Hunt & Reffert	2024	–	–	–	–	–	907*	–	–
Cavallo et al.	2024	1.61	1.67	–	26	0.310	–	–	–
He et al.	2023	1.86	2.95	–	3	–	–	–	–
Hunt & Reffert	2023	1.69	2.43	2.57	5	–	–	–	–
Almeida et al.	2023	1.56	2.45	–	6	0.051	391*	0.59	–
Just et al.	2023	–	–	–	25	–	52	–	–
Dias et al.	2021	1.46	2.36	–	9	-0.029	–	–	–
Loktin & Popova	2017	2.18	1.95	–	120	–	–	–	–
Kharchenko et al.	2016	1.59	2.84	–	25	–	–	–	–
Kharchenko et al.	2013	1.59	2.84	–	25	–	–	–	–
Dias et al.	2002	1.59	2.84	–	25	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 305	0.7	304.33	39.63	0.36	-3.57	-5.43	–	0.12

💡 Note: The % column shows the percentage of members that VDB 130 shares with each listed object.

Visualization

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