VDBH 79

(vdBergh-Hagen 79; MWSC 1708; BH 79)

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0.55 UTI
0.36
CN
1.0
Cdens
0.5
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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VDBH 79 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as an extremely massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.43 kpc) differs significantly from the median photometric distance (~6.64 kpc).

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Very distant High extinction Extremely massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Dias et al. (2002)
Asterism (Bica, E.; Bonatto, C. 2011, A&A 530, 32)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 146.119 -53.28 0.291 -4.53 3.342 –
Hunt & Reffert 2024 146.163 -53.275 0.289 -4.534 3.36 –
Cavallo et al. 2024 146.147 -53.282 0.288 – – –
Hunt & Reffert 2023 146.163 -53.275 0.289 -4.534 3.36 –
Just et al. 2023 146.026 -53.321 – – – –
Bica et al. 2019 145.923 -53.249 – – – –
Kharchenko et al. 2016 146.026 -53.321 – – – –
Kharchenko et al. 2013 146.032 -53.325 – -7.17 3.53 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 446* – –
Cavallo et al. 2024 2.91 3.29 – 151 0.180 – – –
Hunt & Reffert 2023 3.01 3.14 2.18 87 – – – –
Just et al. 2023 – – – 251 – 31261 – –
Kharchenko et al. 2016 10.27 4.26 – 251 – – – –
Kharchenko et al. 2013 10.27 4.26 – 251 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2646 75.0 146.15 -53.28 0.29 -4.55 3.35 – 0.14

💡 Note: The % column shows the percentage of members that VDBH 79 shares with each listed object.

Visualization

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