VDBH 72

(FSR 1494; vdBergh-Hagen 72; BH 72; ESO 166 20; MWSC 1681)

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C3
N_50
r_50
AB 177 1.9
Summary

VDBH 72 is a rich, very dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is well-studied in the literature.

This object shares a moderate percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 142.85 -53.05 -2.75 9.98
Froebrich et al. (2007) 142.858 -53.028
Kharchenko et al. (2012) 142.845 -53.035 -5.37 2.02
Cantat-Gaudin et al. (2018) 142.838 -53.04 0.11 -4.621 3.299
Bica et al. (2019) 142.845 -53.034
Soubiran et al. (2018) 142.838 -53.04 50.74
Cantat-Gaudin et al. (2020) 142.838 -53.04 0.11 -4.621 3.299
Dias et al. (2021) 142.843 -53.041 0.094 -4.648 3.297 50.334
Hunt & Reffert (2023) 142.842 -53.042 0.175 -4.53 3.354 52.388
Cavallo et al. (2024) 142.853 -53.028 0.176
Hunt & Reffert (2024) 142.842 -53.042 0.175 -4.53 3.354 52.388
Almeida et al. (2025) 142.843 -53.041
           
UCC 142.849 -53.04 0.146 -4.581 3.34 50.03
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.48, Dist=3190.0, Age=9.1
Kharchenko et al. (2012) e_bv=0.5, distance=2032, log_age=8.7
Cantat-Gaudin et al. (2018) dmode=7181.9
Soubiran et al. (2018) dmode=7181.9
Cantat-Gaudin et al. (2020) AVNN=2.53, DistPc=5844.0, AgeNN=8.35
Dias et al. (2021) Av=2.529, Dist=4289, logage=8.848, [Fe/H]=-0.056
Hunt & Reffert (2023) AV50=2.738, diffAV50=1.723, MOD50=13.419, logAge50=8.234
Cavallo et al. (2024) AV50=2.87, dMod50=13.29, logAge50=8.2, [Fe/H]50=0.32
Hunt & Reffert (2024) MassJ=1977.05, MassTot=1977.05
Almeida et al. (2025) AV=2.529, Dist=4289, logAge=8.848, MassRk=754.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0516 28.2 142.85 -53.04 0.16 -4.58 3.34 50.0 0.0
UBC 491 28.2 142.86 -53.02 0.22 -4.46 3.34 49.91 0.29