Berkeley 48

(NGC 6827; MWSC 3186; OCL 120; FSR 0152)

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0.88 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad) 19.6 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.81 Well-studied
  • Cdup 1.0 Unique

Overview

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Berkeley 48 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 moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~9.23 kpc) differs significantly from the median photometric distance (~6.47 kpc).

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 297.221 21.214 0.108 -2.453 -5.465 -8.165
Almeida et al. 2025 297.22 21.214 – – – –
Hunt & Reffert 2024 297.222 21.214 0.124 -2.462 -5.456 -1.635
Cavallo et al. 2024 297.225 21.207 0.119 – – –
Hunt & Reffert 2023 297.222 21.214 0.124 -2.462 -5.456 -1.635
Just et al. 2023 297.208 21.213 – – – –
Dias et al. 2021 297.22 21.214 0.095 -2.408 -5.465 –
Cantat-Gaudin et al. 2020 297.22 21.213 0.103 -2.418 -5.465 –
SΓ‘nchez et al. 2020 297.221 21.215 – -2.273 -5.454 –
Cantat-Gaudin & Anders 2020 297.22 21.213 0.103 -2.418 -5.465 –
Soubiran et al. 2018 297.22 21.213 – – – 23.75
Bica et al. 2019 297.227 21.22 – – – –
Cantat-Gaudin et al. 2018 297.22 21.213 0.103 -2.418 -5.465 –
Kharchenko et al. 2016 297.208 21.213 – – – –
Kharchenko et al. 2013 297.213 21.215 – 1.4 -12.34 –
Dias et al. 2002 297.221 21.215 – 1.92 -5.07 –

πŸ’‘ 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– 6.47 2.595 2.33 955 -0.224 1632 – –
Almeida et al. 2025 6.47 2.36 – 853 – 1632 – –
Hunt & Reffert 2024 – – – – – 3054(1) – –
Cavallo et al. 2024 5.27 3.42 – 331 -0.700 – – –
Hunt & Reffert 2023 7.04 3.18 2.33 226 – – – –
Just et al. 2023 – – – 1148 – 372 – –
Dias et al. 2021 6.47 2.36 – 853 0.253 – – –
Cantat-Gaudin et al. 2020 5.73 1.98 – 1288 – – – –
Cantat-Gaudin & Anders 2020 7.59 – – – – – – –
Soubiran et al. 2018 7.59 – – – – – – –
Cantat-Gaudin et al. 2018 7.59 – – – – – – –
Kharchenko et al. 2016 4.19 2.77 – 1148 – – – –
Kharchenko et al. 2013 4.19 2.77 – 1148 – – – –
Dias et al. 2002 4.55 2.42 – 955 – – – –

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

Visualization

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