VDBH 253

(Czernik 37; OCL 8; vdBergh-Hagen 253; ESO 521 03; MWSC 2737; FoF 284)

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C3
N_50
r_50
AA 343 2.4
Summary

VDBH 253 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 268.321 -27.369 0.74 -3.72
Kharchenko et al. (2012) 268.32 -27.365 -0.28 -1.24
Cantat-Gaudin et al. (2018) 268.32 -27.373 0.406 0.459 -0.445
Bica et al. (2019) 268.317 -27.37
Soubiran et al. (2018) 268.32 -27.373 -19.21
Liu & Pang (2019) 268.321 -27.368 0.425 0.463 -0.439
Cantat-Gaudin et al. (2020) 268.32 -27.373 0.406 0.459 -0.445
Dias et al. (2021) 268.322 -27.376 0.399 0.449 -0.426 -19.527
Hunt & Reffert (2023) 268.318 -27.366 0.371 0.462 -0.465 -2.124
Cavallo et al. (2024) 268.321 -27.37 0.37
Hunt & Reffert (2024) 268.318 -27.366 0.371 0.462 -0.465 -2.124
Almeida et al. (2025) 268.322 -27.376
           
UCC 268.319 -27.374 0.376 0.455 -0.463 -19.193
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)=1.47, Dist=1440.0, Age=8.4
Kharchenko et al. (2012) e_bv=1.208, distance=1668, log_age=8.77
Cantat-Gaudin et al. (2018) dmode=2298.2
Soubiran et al. (2018) dmode=2298.2
Liu & Pang (2019) Age=0.407, Z=0.0
Cantat-Gaudin et al. (2020) AVNN=3.43, DistPc=2314.0, AgeNN=8.58
Dias et al. (2021) Av=3.604, Dist=1872, logage=8.56, [Fe/H]=0.483
Hunt & Reffert (2023) AV50=4.952, diffAV50=2.535, MOD50=11.945, logAge50=8.015
Cavallo et al. (2024) AV50=5.06, dMod50=11.48, logAge50=7.4, [Fe/H]50=-0.75
Hunt & Reffert (2024) MassJ=5867.77, MassTot=5867.77
Almeida et al. (2025) AV=3.604, Dist=1872, logAge=8.56, MassRk=1821.5

Search coordinates in Bayestar19

Cluster region map