Collinder 419

(MWSC 3305)

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0.91 UTI
0.8
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 31.5 [N/pc2]
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Collinder 419 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Cavallo et al. (2024)
Silver sample.

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. 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– 304.589 40.789 0.974 -2.687 -6.372 -5.638
Wei et al. 2025 304.876 40.888 0.978 -2.576 -6.335 –
Almeida et al. 2025 304.532 40.747 – – – –
Hunt & Reffert 2024 304.527 40.726 0.972 -2.558 -6.355 -7.648
Celli et al. 2024 304.534 40.732 – – – –
Cavallo et al. 2024 304.81 40.85 0.974 – – –
Hunt & Reffert 2023 304.527 40.726 0.972 -2.558 -6.355 -7.648
Almeida et al. 2023 304.534 40.743 – – – –
Just et al. 2023 304.525 40.723 – – – –
He et al. 2022 304.802 40.877 0.978 -2.573 -6.352 –
Dias et al. 2021 304.532 40.747 0.958 -2.704 -6.284 9.371
Cantat-Gaudin et al. 2020 304.534 40.732 0.952 -2.708 -6.382 –
Cantat-Gaudin & Anders 2020 304.534 40.732 0.952 -2.708 -6.382 –
Soubiran et al. 2018 304.534 40.732 – – – 4.64
Cantat-Gaudin et al. 2018 304.534 40.732 0.952 -2.708 -6.382 –
Loktin & Popova 2017 304.53 40.732 – -1.017 -1.279 -8.3
Kharchenko et al. 2016 304.525 40.723 – – – –
Dias et al. 2014 304.529 40.732 – -2.15 -6.28 –
Kharchenko et al. 2013 304.53 40.725 – -2.21 -6.31 -8.3
Gozha et al. 2012 304.529 40.732 – – – –
Piskunov et al. 2008 304.498 40.714 – – – –
Kharchenko et al. 2007 304.53 40.73 – 0.25 – -8.3
Kharchenko et al. 2005 304.5 40.72 – -2.56 -6.99 -8.19
Kharchenko et al. 2003 304.5 40.72 – -2.76 -6.99 –
Dias et al. 2002 304.529 40.732 – -2.15 -6.28 -8.22

💡 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– 1.0 1.13 2.95 7 -0.022 155 0.435 –
Wei et al. 2025 1.00 2.00 – 4 0.000 1026 0.48 –
Almeida et al. 2025 1.00 1.13 – 6 – 174 – –
Hunt & Reffert 2024 – – – – – 1307(1) – –
Celli et al. 2024 – – – 20 – 143 – –
Cavallo et al. 2024 1.02 1.99 – 4 -0.090 – – –
Hunt & Reffert 2023 1.00 2.38 2.95 5 – – – –
Almeida et al. 2023 0.99 1.24 – 5 -0.044 155(1) 0.39 –
Just et al. 2023 – – – 13 – 95 – –
He et al. 2022 – 2.05 – 4 – – – –
Dias et al. 2021 1.00 1.13 – 6 0.091 – – –
Cantat-Gaudin et al. 2020 1.00 1.17 – 19 – – – –
Cantat-Gaudin & Anders 2020 1.02 – – – – – – –
Soubiran et al. 2018 1.02 – – – – – – –
Cantat-Gaudin et al. 2018 1.02 – – – – – – –
Loktin & Popova 2017 1.74 2.97 – 35 – – – –
Kharchenko et al. 2016 0.87 0.97 – 13 – – – –
Kharchenko et al. 2013 0.87 0.97 – 13 – – – –
Gozha et al. 2012 0.77 – – 7 – 148 – –
Piskunov et al. 2008 0.74 1.05 – 7 – – – –
Kharchenko et al. 2005 0.74 1.05 – 7 – – – –
Kharchenko et al. 2003 0.77 0.93 – – – – – –
Dias et al. 2002 0.74 1.05 – 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0223 7.6 304.9 40.92 0.97 -2.46 -6.3 -15.71 0.37

💡 Note: The % column shows the percentage of members that Collinder 419 shares with each listed object.

Visualization

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