Berkeley 88

(MWSC 3323)

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0.51 UTI
0.57
CN
1.0
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 16.0 [N/pc2]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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Berkeley 88 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a large* distance, well above the mid-plane, affected by high extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~8.65 kpc) differs significantly from the median photometric distance (~5.68 kpc).

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 305.308 48.141 0.116 -3.973 -4.659 -68.164
Just et al. 2023 305.329 48.137 – – – –
Kharchenko et al. 2016 305.329 48.137 – – – –
Kharchenko et al. 2013 305.332 48.14 – -2.49 -4.02 –
Bukowiecki et al. 2011 305.304 48.139 – – – –
Dias et al. 2002 305.4 48.083 – -2.49 -4.02 –

💡 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– 5.68 3.235 – 653 – 1538 – –
Just et al. 2023 – – – 653 – 1538 – –
Kharchenko et al. 2016 5.04 3.74 – 653 – – – –
Kharchenko et al. 2013 5.04 3.74 – 653 – – – –
Bukowiecki et al. 2011 8.95(1) 2.67 – 1585 – – – –
Dias et al. 2002 6.32 2.73 – 1585 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3863 72.3 305.3 48.14 0.11 -3.96 -4.65 -68.16 0.06

💡 Note: The % column shows the percentage of members that Berkeley 88 shares with each listed object.

Visualization

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