Collinder 333

(MWSC 2618; OCL 1017; ESO 393 04)

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0.69 UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad) 5.5 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.62 Moderately studied
  • Cdup 1.0 Unique

Overview

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Collinder 333 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~2.59 kpc) differs significantly from the median photometric distance (~1.05 kpc).

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

Cavallo et al. (2024)
Wood 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– 262.85 -34.003 0.386 0.055 -1.092 -23.739
Hunt & Reffert 2024 262.788 -33.998 0.398 0.023 -1.103 64.058
Cavallo et al. 2024 262.822 -33.999 0.397 – – –
Hunt & Reffert 2023 262.788 -33.998 0.398 0.023 -1.103 64.058
Just et al. 2023 262.895 -34.01 – – – –
Bica et al. 2019 262.869 -34.023 – – – –
Kharchenko et al. 2016 262.895 -34.01 – – – –
Dias et al. 2014 262.879 -34.017 – -2.42 0.38 –
Kharchenko et al. 2013 262.905 -34.01 – 0.71 -2.25 –
Piskunov et al. 2008 262.869 -34.023 – – – –
Kharchenko et al. 2005 262.87 -34.02 – 0.68 -4.88 –
Dias et al. 2002 262.879 -34.017 – -2.42 0.38 –

💡 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– 1.05 3.29 3.02 141 -1.640 688 – –
Hunt & Reffert 2024 – – – – – 1348(1) – –
Cavallo et al. 2024 1.39 5.34 – 1 -1.640 – – –
Hunt & Reffert 2023 2.34 4.70 3.02 5 – – – –
Just et al. 2023 – – – 141 – 27 – –
Kharchenko et al. 2016 1.05 3.29 – 141 – – – –
Kharchenko et al. 2013 1.05 3.29 – 141 – – – –
Piskunov et al. 2008 0.85 0.34 – 794 – – – –
Kharchenko et al. 2005 0.85 0.34 – 794 – – – –
Dias et al. 2002 0.85 0.34 – 794 – – – –

(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 1798 65.1 262.84 -34.0 0.38 0.09 -1.07 -39.26 0.03

💡 Note: The % column shows the percentage of members that Collinder 333 shares with each listed object.

Visualization

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