Collinder 471

(MWSC 3587)

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0.63 UTI
0.27
CN
1.0
Cdens
1.0
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 14.1 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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Collinder 471 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close* distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~0.34 kpc) differs significantly from the median photometric distance (~2.00 kpc).

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Cantat-Gaudin et al. (2020)
Catalogue parameters are highly discrepant. No clear radius or kinematic signature identified. More details in Appendix A of the article.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 332.562 73.025 2.923 5.334 1.565 -17.775
Cavallo et al. 2024 333.393 73.346 2.928 – – –
Hunt & Reffert 2023 332.563 73.032 2.93 5.321 1.632 -22.556
Just et al. 2023 331.682 71.972 – – – –
Kharchenko et al. 2016 331.682 71.972 – – – –
Dias et al. 2014 331.775 72.0 – -2.22 -3.32 -10.94
Kharchenko et al. 2013 331.687 71.975 – 4.09 -2.09 –
Kharchenko et al. 2012 331.702 71.978 – 3.09 -2.81 –
Dias et al. 2002 331.775 72.0 – -2.22 -3.32 -10.94

💡 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– 2.0 3.1 1.39 8 0.140 427 – –
Cavallo et al. 2024 0.34 1.64 – 5 0.140 – – –
Hunt & Reffert 2023 0.33 0.75 1.39 5 – – – –
Just et al. 2023 – – – 631 – 427 – –
Kharchenko et al. 2016 2.21 3.16 – 631 – – – –
Kharchenko et al. 2013 2.21 3.16 – 631 – – – –
Kharchenko et al. 2012 2.00 3.10 – 8 – – – –
Dias et al. 2002 2.00 3.10 – 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 38 100.0 332.89 73.15 2.93 5.36 1.58 -17.5 0.01
Theia 10 100.0 333.13 73.25 2.93 5.4 1.58 -16.15 0.24

💡 Note: The % column shows the percentage of members that Collinder 471 shares with each listed object.

Visualization

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