VDBH 60

(BH 60)

0.00 UTI

0.64

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 78

Stellar density (N₅₀/rad) 88.8 [N/pc²]

C3 classification AA

C_N 0.64 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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VDBH 60 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 12 years.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~2.69 kpc) differs significantly from the median photometric distance (~1325.00 kpc).

Extremely distant Moderate extinction Intermediate age

Data

🔍 Search references for VDBH 60 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–	138.97	-50.007	0.372	-5.346	3.984	-4.758
Tadross	2014	138.971	-50.011	–	–	–	–

💡 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–	1325.0	2.08	–	400	–	–	–	–
Tadross	2014	1325.00	2.08	–	400	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Pismis 11	100.0	138.97	-50.0	0.37	-5.34	3.98	61.2	0.86

💡 Note: The % column shows the percentage of members that VDBH 60 shares with each listed object.

Visualization

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