VDBH 90

(vdBergh-Hagen 90; BH 90; FoF 124)

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C3
N_50
r_50
AA 220 2.3
Summary

VDBH 90 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 153.042 -58.067 -0.22 2.86
Kharchenko et al. (2012) 153.045 -58.06 -1.69 3.14
Cantat-Gaudin et al. (2018) 153.064 -58.069 0.369 -5.385 2.295
Liu & Pang (2019) 153.096 -58.068 0.367 -5.456 2.473
Cantat-Gaudin et al. (2020) 153.064 -58.069 0.369 -5.385 2.295
Dias et al. (2021) 153.07 -58.07 0.352 -5.386 2.309
Hunt & Reffert (2023) 153.052 -58.075 0.374 -5.409 2.35 25.524
Cavallo et al. (2024) 153.081 -58.067 0.375
Hunt & Reffert (2024) 153.052 -58.075 0.374 -5.409 2.35 25.524
Almeida et al. (2025) 153.07 -58.07
           
UCC 153.062 -58.072 0.375 -5.405 2.327 25.531
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.526, Dist=2572.0, Age=7.943
Kharchenko et al. (2012) e_bv=0.541, distance=1928, log_age=8.465
Cantat-Gaudin et al. (2018) dmode=2513.6
Liu & Pang (2019) Age=0.11, Z=-0.5
Cantat-Gaudin et al. (2020) AVNN=1.39, DistPc=2792.0, AgeNN=8.1
Dias et al. (2021) Av=1.785, Dist=2294, logage=8.312, [Fe/H]=-0.016
Hunt & Reffert (2023) AV50=1.974, diffAV50=2.392, MOD50=11.931, logAge50=7.848
Cavallo et al. (2024) AV50=1.85, dMod50=11.7, logAge50=8.36, [Fe/H]50=0.09
Hunt & Reffert (2024) MassJ=1034.74, MassTot=1063.56
Almeida et al. (2025) AV=1.785, Dist=2294, logAge=8.312, MassRk=662.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Bochum 8 100.0 153.06 -58.07 0.38 -5.4 2.34 26.8 0.52