NGC 2244

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0.93 UTI
0.9
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Core radius and density 0.5 [pc], 38 [pc-2]
  • CN 0.9 Very rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 2244 is a very rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (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.

Li et al. (2026)
Tidal & Core radii: r_t=43+/-15.5 [pc], r_c=0.44+/-0.0 [pc]; stars within r_t: N~473

Liu et al. (2025)
Classified as primordial binary cluster 281 along with HSC_1629, and of multiple system 42 along with Collinder_106, Collinder_107 and HSC_1629.

Palma et al. (2025)
Part of multiple system G20, along with HSC_1629, Desvoivres_2, Collinder_107 and Collinder_106.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.88 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.88 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.1343, e_all=0.1035.

Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg19' along with Collinder 106 and Collinder 107.

Lada & Lada (2003)
Embedded cluster within âˆŧ2 Kpc of the Sun.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 98.012 4.908 0.653 -1.708 0.234 27.148
Li et al. 2026 98.06 4.89 – – – –
Otto et al. 2026 97.985 4.927 – -1.6 0.18 34.3
Liu et al. 2025 97.99 4.93 0.66 -1.74 0.25 31.88
Schweers & McSwain 2026 98.04 4.9 – – – –
Yang et al. 2025 97.985 4.927 – – – –
Almeida et al. 2025 98.088 4.917 – – – –
Zhang et al. 2024 97.985 4.927 – – – –
Hunt & Reffert 2024 97.985 4.927 0.657 -1.737 0.253 31.885
Celli et al. 2024 98.045 4.914 – – – –
Cavallo et al. 2024 97.993 4.905 0.659 – – –
Hunt & Reffert 2023 97.985 4.927 0.657 -1.737 0.253 31.885
Fu et al. 2022 98.045 4.914 – – – 23.481
Jaehnig et al. 2021 98.029 4.917 0.681 -1.734 0.221 –
Rain et al. 2021 98.045 4.914 0.617 -1.598 0.179 –
Richer et al. 2021 98.085 4.875 0.648 -1.581 0.155 –
Dias et al. 2021 98.088 4.917 0.605 -1.563 0.186 92.271
Cantat-Gaudin et al. 2020 98.045 4.914 0.617 -1.598 0.179 –
Zhong et al. 2020 98.045 4.914 – -1.598 0.179 31.758
Cantat-Gaudin & Anders 2020 98.045 4.914 0.617 -1.598 0.179 –
Dias et al. 2019 98.046 4.914 0.617 -1.598 0.179 102.43
Soubiran et al. 2018 98.045 4.914 – – – 75.18
Cantat-Gaudin et al. 2018 98.045 4.914 0.617 -1.598 0.179 –
Dias et al. 2018 – – – -2.03 -0.62 –
Dib et al. 2018 97.98 4.94 – – – –
Loktin & Popova 2017 97.98 4.942 – -0.04 -1.04 26.2
Sampedro et al. 2017 97.979 4.942 – -0.65 -1.36 –
Joshi et al. 2016 97.98 4.94 – – – –
Dias et al. 2016 97.979 4.942 – -0.65 0.67 30.67
Dias et al. 2014 97.979 4.942 – -0.23 -1.13 –
Gozha et al. 2012 97.979 4.942 – – – –
Bukowiecki et al. 2011 97.992 4.94 – – – –
Kharchenko et al. 2009 97.969 4.943 – – – –
Piskunov et al. 2008 97.969 4.943 – – – –
Kharchenko et al. 2007 97.98 4.94 – 0.32 – 26.16
Piskunov et al. 2007 97.969 4.943 – – – –
Ahumada & Lapasset 2007 97.975 4.95 – – – –
van den Bergh 2006 97.975 4.933 – – – –
Kharchenko et al. 2005 97.98 4.94 – -1.42 -0.32 26.16
Lada & Lada 2003 98.73 4.42 – – – –
Kharchenko et al. 2003 97.99 4.94 – -0.95 -0.3 –
Chen et al. 2003 98.087 4.891 – -0.65 0.67 36.6
Dias et al. 2002 97.979 4.942 – -0.65 0.67 36.6
Dambis 1999 97.979 4.942 – – – –
Lynga 1987 98.078 4.864 – – – 33.0
Sulentic et al. 1973 98.082 4.864 – – – –
Alter et al. 1970 98.078 4.864 – – – –

💡 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– 1.45 1.46 2.43 5 -0.196 1120 – 0
Otto et al. 2026 – – – 13 0.020(15) – – –
Liu et al. 2025 2.04 0.46 – 11 – – – –
Schweers & McSwain 2026 1.35 – – 8 – – – –
Yang et al. 2025 – – – 4 -0.330(3) – – –
Almeida et al. 2025 1.25 1.57 – 13 – 705 – –
Zhang et al. 2024 – – – – -0.127(1) – – –
Hunt & Reffert 2024 1.42 1.63 2.43 4 – 1388(1) – –
Celli et al. 2024 – – – 13 – 2097 – –
Cavallo et al. 2024 1.24 1.28 – 4 0.260 – – –
Hunt & Reffert 2023 1.42 1.63 2.43 4 – – – –
Fu et al. 2022 – – – – -0.076 – – –
Jaehnig et al. 2021 1.45(1) – – – – – – –
Rain et al. 2021 1.55 1.48 – 2 – – – 0
Richer et al. 2021 – 2.22 – – – – – –
Dias et al. 2021 1.25 1.57 – 13 -0.214 – – –
Cantat-Gaudin et al. 2020 1.48 1.46 – 13 – – – –
Kounkel et al. 2020 1.70 2.48 – 5 – – – –
Zhong et al. 2020 1.55(1) – – – -0.177 – – –
Cantat-Gaudin & Anders 2020 1.55 – – – – – – –
Dias et al. 2019 1.30 1.39 – 8 -0.483 – – –
Soubiran et al. 2018 1.55 – – – – – – –
Cantat-Gaudin et al. 2018 1.55 – – – – – – –
Dib et al. 2018 1.53 – – 5 – – – –
Loktin & Popova 2017 1.45 1.46 – 8 – – – –
Joshi et al. 2016 1.53 1.71 – 5 – 851 – –
Dias et al. 2016 1.66 1.48 – 2 – – – –
Bukowiecki et al. 2012 – – – – – 3834 – –
Gozha et al. 2012 1.45 – – 2 -0.460 851 – –
Bukowiecki et al. 2011 1.20(1) 1.70 – 7 – – – –
Paunzen et al. 2010 – – – – -0.460 – – –
Kharchenko et al. 2009 1.45 1.26 – 5 – – – –
Piskunov et al. 2008 1.45 1.26 – 5 – 1422(1) – –
Piskunov et al. 2007 1.45 1.26 – 5 – 354 – –
Ahumada & Lapasset 2007 – 1.45 – 8 – – – 0
van den Bergh 2006 1.45 1.45 – 8 – – – –
Kharchenko et al. 2005 1.45 1.26 – 5 – – – –
Lada & Lada 2003 1.60 – – – – – – –
Kharchenko et al. 2003 1.45 1.26 – – – – – –
Chen et al. 2003 1.45 – – 0 – – – –
Dias et al. 2002 1.45 1.46 – 8 – – – –
Dambis 1999 1.43 1.53 – 3 – – – –
Lynga 1987 1.70 1.42 – 3 – – – –
Alter et al. 1970 1.70 – – – – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 2239 3.1 97.76 4.94 0.67 -1.83 0.03 24.06 0.5

💡 Note: The % column shows the percentage of members that NGC 2244 shares with each listed object.

Visualization

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