Collinder 417

(NGC 6885; MWSC 3282; 20 Vul; OCL 132)

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0.58 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad) 8.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.69 Moderately studied
  • Cdup 1.0 Unique

Overview

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Collinder 417 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~1.79 kpc) differs significantly from the median photometric distance (~1.02 kpc).

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

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 302.92 26.501 0.559 -3.155 -5.54 85.771
Almeida et al. 2025 302.983 26.494 – – – –
Just et al. 2023 303.002 26.512 – – – –
Dias et al. 2021 302.983 26.494 0.439 -3.127 -5.471 2.378
SΓ‘nchez et al. 2020 303.004 26.478 – -3.145 -5.666 –
Bica et al. 2019 303.001 26.481 – – – –
Loktin & Popova 2017 303.0 26.478 – -3.3 -5.14 -1.5
Kharchenko et al. 2016 303.002 26.512 – – – –
Dias et al. 2014 303.004 26.478 – -3.3 -5.14 –
Kharchenko et al. 2013 303.007 26.515 – -1.0 -3.79 -1.5
Gozha et al. 2012 303.004 26.478 – – – –
van den Bergh 2006 303.0 26.483 – – – –
Dias et al. 2002 303.004 26.478 – -3.3 -5.14 -1.5

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– 1.025 1.93 – 1109 0.055 1848 – –
Almeida et al. 2025 1.45 1.93 – 124 – 866 – –
Just et al. 2023 – – – 1109 – 2831 – –
Dias et al. 2021 1.45 1.93 – 124 0.055 – – –
Loktin & Popova 2017 0.44 0.46 – 462 – – – –
Kharchenko et al. 2016 3.78 3.03 – 1109 – – – –
Kharchenko et al. 2013 3.78 3.03 – 1109 – – – –
Gozha et al. 2012 0.60 – – 1445 – – – –
van den Bergh 2006 0.60 0.25 – 1445 – – – –
Dias et al. 2002 0.60 0.25 – 1445 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 18 84.0 302.91 26.54 0.61 -3.21 -5.66 -3.42 0.79

πŸ’‘ Note: The % column shows the percentage of members that Collinder 417 shares with each listed object.

Visualization

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