VDBH 106

(van den Bergh-Hagen 106; BH 106; vdBergh-Hagen 106; MWSC 1863)

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0.17 UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.29
Clit
1.0
Cdup
Core radius and density 5.1 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.25 Low quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
VDBH 106 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.00 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 163.14 -54.247 0.368 -7.471 2.514 7.536
Hunt & Reffert 2023 163.349 -54.248 0.376 -7.485 2.51 –
Just et al. 2023 163.15 -54.261 – – – –
Bica et al. 2019 163.186 -54.269 – – – –
Sampedro et al. 2017 163.175 -54.233 – -5.54 -0.42 –
Kharchenko et al. 2016 163.15 -54.261 – – – –
Dias et al. 2014 163.175 -54.233 – -6.88 0.74 –
Kharchenko et al. 2013 163.158 -54.265 – -8.33 4.66 –
Bukowiecki et al. 2011 163.167 -54.262 – – – –
Dias et al. 2002 163.175 -54.233 – -6.88 0.74 –
Lynga 1987 163.185 -54.247 – – – –
van den Bergh & Hagen 1975 162.65 -53.983 – – – –

💡 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] Bfrac BSS
UCC 99999– 2.785 1.15 1.09 1841 – 865 – –
Hunt & Reffert 2023 2.43 0.45 1.09 8110 – – – –
Just et al. 2023 – – – 1841 – 865 – –
Kharchenko et al. 2016 3.14 1.15 – 1841 – – – –
Kharchenko et al. 2013 3.14 1.15 – 1841 – – – –
Dias et al. 2002 1.88 1.28 – 100 – – – –

Visualization

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