VDBH 150

(van den Bergh-Hagen 150; vdBergh-Hagen 150; MWSC 2143; BH 150)

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0.73 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.45
Clit
1.0
Cdup
Nm (P>50%) 111
Core radius and density 1.4 [pc], 6.5 [pc-2]
C3 classification AA
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
VDBH 150 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is poorly studied in the literature.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.14 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.14 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.0873, e_all=0.1273.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Dias et al. (2002)
No cluster (Carraro, G.; Janes, K. A.; Eastman, J. D. 2005, MNRAS 364, 179); cat V3.5 (Jan 2016)

Data
🔍 Search references for VDBH 150 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 204.507 -63.348 0.2 -6.394 -1.532 -26.303
Hunt & Reffert 2024 204.517 -63.344 0.219 -6.406 -1.528 87.85
Celli et al. 2024 204.506 -63.346 – – – –
Cavallo et al. 2024 204.481 -63.352 0.217 – – –
Hunt & Reffert 2023 204.517 -63.344 0.219 -6.406 -1.528 87.85
Just et al. 2023 204.461 -63.317 – – – –
Cantat-Gaudin et al. 2020 204.506 -63.346 0.178 -6.395 -1.534 –
Cantat-Gaudin & Anders 2020 204.506 -63.346 0.178 -6.395 -1.534 –
Soubiran et al. 2018 204.506 -63.346 – – – -41.95
Cantat-Gaudin et al. 2018 204.506 -63.346 0.178 -6.395 -1.534 –
Dib et al. 2018 204.472 -63.32 – – – –
Joshi et al. 2016 204.472 -63.32 – – – –
Kharchenko et al. 2016 204.461 -63.317 – – – –
Kharchenko et al. 2013 204.472 -63.32 – -11.9 -3.59 –
Lynga 1987 204.459 -63.334 – – – –
van den Bergh & Hagen 1975 203.6 -63.083 – – – –

💡 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– 3.96 3.895 2.8 32 0.020 582 – –
Hunt & Reffert 2024 4.47 4.47 2.80 63 – 2745(1) – –
Celli et al. 2024 – – – 22 – 582 – –
Cavallo et al. 2024 2.73 4.42 – 195 0.020 – – –
Hunt & Reffert 2023 4.47 4.47 2.80 63 – – – –
Just et al. 2023 – – – 32 – 68 – –
Cantat-Gaudin et al. 2020 5.57 3.76 – 22 – – – –
Kounkel et al. 2020 3.45 4.03 – 47 – – – –
Cantat-Gaudin & Anders 2020 4.84 – – – – – – –
Soubiran et al. 2018 4.84 – – – – – – –
Cantat-Gaudin et al. 2018 4.84 – – – – – – –
Dib et al. 2018 1.54 – – 32 – – – –
Joshi et al. 2016 1.54 0.66 – 32 – – – –
Kharchenko et al. 2016 1.54 0.66 – 32 – – – –
Kharchenko et al. 2013 1.54 0.66 – 32 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization
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VDBH 150 UCC
VDBH 150 HUNT23
VDBH 150 CANTAT20
Galactocentric position diagram