VDBH 211

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

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C3
N_50
r_50
AB 209 5.6
Summary

VDBH 211 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 255.546 -41.1 -3.45 -3.13
Kharchenko et al. (2012) 255.546 -41.11 -1.48 -2.29
Cantat-Gaudin et al. (2018) 255.535 -41.113 0.524 -0.671 -1.943
Bica et al. (2019) 255.549 -41.109
Soubiran et al. (2018) 255.535 -41.113 -48.83
Donor et al. (2020) 255.546 -41.1 -0.68 -2.04 -49.0
Cantat-Gaudin et al. (2020) 255.535 -41.113 0.524 -0.671 -1.943
Dias et al. (2021) 255.541 -41.124 0.51 -0.669 -1.951 -48.896
Hunt & Reffert (2023) 255.527 -41.112 0.572 -0.71 -1.923 -53.127
Cavallo et al. (2024) 255.518 -41.124 0.57
Hunt & Reffert (2024) 255.527 -41.112 0.572 -0.71 -1.923 -53.127
Almeida et al. (2025) 255.541 -41.124
Hu & Soubiran (2025) 255.518 -41.124
           
UCC 255.522 -41.121 0.553 -0.695 -1.947 -48.342
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)=0.61, Dist=1440.0, Age=9.0
Kharchenko et al. (2012) e_bv=1.072, distance=1820, log_age=8.52
Cantat-Gaudin et al. (2018) dmode=1808.6
Soubiran et al. (2018) dmode=1808.6
Donor et al. (2020) Fe/H=0.21
Cantat-Gaudin et al. (2020) AVNN=2.18, DistPc=1903.0, AgeNN=8.63
Dias et al. (2021) Av=2.388, Dist=1638, logage=8.825, [Fe/H]=0.124
Hunt & Reffert (2023) AV50=2.634, diffAV50=2.041, MOD50=11.085, logAge50=8.234
Cavallo et al. (2024) AV50=2.85, dMod50=10.71, logAge50=8.83, [Fe/H]50=-0.25
Hunt & Reffert (2024) MassJ=1077.60, MassTot=1077.60
Almeida et al. (2025) AV=2.388, Dist=1638, logAge=8.825, MassRk=557.5
Hu & Soubiran (2025) MA22=-0.22, MA23f=-0.09, MA23g=0.21, MZ23=-0.4, MK24=-0.12, MF24=-0.31

Search coordinates in Bayestar19

Cluster region map