Berkeley 100

(MWSC 3727; OCL 264)

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0.80 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad) 10.8 [N/pc2]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique

Overview

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Berkeley 100 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, above 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 well-studied in the literature.

(*): The parallax distance estimate (~6.08 kpc) differs significantly from the median photometric distance (~4.30 kpc).

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– 351.484 63.779 0.165 -3.267 -1.475 -65.069
Hunt & Reffert 2024 351.489 63.78 0.173 -3.265 -1.459 -45.808
Cavallo et al. 2024 351.502 63.784 0.172 – – –
Hunt & Reffert 2023 351.489 63.78 0.173 -3.265 -1.459 -45.808
Just et al. 2023 351.468 63.775 – – – –
Cantat-Gaudin et al. 2020 351.485 63.781 0.123 -3.372 -1.557 –
SΓ‘nchez et al. 2020 351.492 63.78 – -3.207 -1.595 –
Cantat-Gaudin & Anders 2020 351.485 63.781 0.123 -3.372 -1.557 –
Bica et al. 2019 351.491 63.782 – – – –
Kharchenko et al. 2016 351.468 63.775 – – – –
Dias et al. 2014 351.492 63.78 – -2.47 -0.26 –
Kharchenko et al. 2013 351.477 63.778 – -1.25 -2.58 –
Kharchenko et al. 2012 351.477 63.778 – -1.25 -2.58 –
Dias et al. 2002 351.492 63.78 – -1.25 -2.58 –

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– 4.305 3.6 2.15 70 -0.350 536 – –
Hunt & Reffert 2024 – – – – – 1052(1) – –
Cavallo et al. 2024 5.45 3.60 – 282 -0.350 – – –
Hunt & Reffert 2023 4.84 3.10 2.15 225 – – – –
Just et al. 2023 – – – 27 – 19 – –
Cantat-Gaudin et al. 2020 6.08 2.48 – 1230 – – – –
Cantat-Gaudin & Anders 2020 6.58 – – – – – – –
Kharchenko et al. 2016 2.70 3.75 – 27 – – – –
Kharchenko et al. 2013 2.70 3.75 – 27 – – – –
Kharchenko et al. 2012 2.70 3.75 – 27 – – – –
Dias et al. 2002 3.77 3.10 – 112 – – – –

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

Visualization

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