Ruprecht 44

(MWSC 1398; OCL 681; ESO 430 05)

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0.95 UTI
0.77
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 8.4 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 44 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, above 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 mass parameter (see Parameters). It is very well-studied in the literature.

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

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

Cavallo et al. (2024)
Gold 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– 119.704 -28.558 0.176 -2.352 2.934 114.157
Li et al. 2025 119.708 -28.558 0.152 -2.381 2.935 –
Almeida et al. 2025 119.713 -28.569 – – – –
Hunt & Reffert 2024 119.692 -28.547 0.181 -2.334 2.917 –
Celli et al. 2024 119.708 -28.558 – – – –
Cavallo et al. 2024 119.697 -28.562 0.181 – – –
Hunt & Reffert 2023 119.692 -28.547 0.181 -2.334 2.917 –
Almeida et al. 2023 119.712 -28.569 – – – –
Just et al. 2023 119.717 -28.583 – – – –
Jaehnig et al. 2021 119.709 -28.563 0.183 -2.366 2.918 –
Rain et al. 2021 119.708 -28.558 0.152 -2.381 2.935 –
Dias et al. 2021 119.713 -28.569 0.156 -2.378 2.938 –
Cantat-Gaudin et al. 2020 119.708 -28.558 0.152 -2.381 2.935 –
Cantat-Gaudin & Anders 2020 119.708 -28.558 0.152 -2.381 2.935 –
Dias et al. 2019 119.713 -28.583 0.172 -2.338 2.843 64.017
Bossini et al. 2019 119.708 -28.558 – – – –
Bica et al. 2019 119.711 -28.566 – – – –
Cantat-Gaudin et al. 2018 119.708 -28.558 0.152 -2.381 2.935 –
Loktin & Popova 2017 119.715 -28.582 – -2.618 -0.892 93.7
Kharchenko et al. 2016 119.717 -28.583 – – – –
Dias et al. 2014 119.713 -28.583 – -2.17 0.17 93.7
Kharchenko et al. 2013 119.722 -28.585 – -1.58 1.02 –
Piskunov et al. 2008 119.707 -28.58 – – – –
van den Bergh 2006 119.725 -28.583 – – – –
Kharchenko et al. 2005 119.71 -28.58 – -5.4 0.17 –
Dias et al. 2002 119.713 -28.583 – -2.17 0.17 93.7
Dambis 1999 119.725 -28.583 – – – –

💡 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– 4.67 1.9 1.87 14 -0.173 1171 0.57 0.0
Li et al. 2025 4.77 1.84 – 22 -0.056 – – –
Almeida et al. 2025 4.50 1.96 – 12 – 34 – –
Hunt & Reffert 2024 – – – – – 1948(1) – –
Celli et al. 2024 – – – 14 – 731 – –
Cavallo et al. 2024 3.58 1.86 – 27 -0.290 – – –
Hunt & Reffert 2023 5.14 1.79 1.87 20 – – – –
Almeida et al. 2023 4.14 1.97 – 16 -0.232 1171(1) 0.57 –
Just et al. 2023 – – – 6 – 3698 – –
Jaehnig et al. 2021 5.53(1) – – – – – – –
Rain et al. 2021 5.54 1.86 – 13 – – – 0
Dias et al. 2021 4.50 1.96 – 12 -0.115 – – –
Cantat-Gaudin et al. 2020 5.75 1.64 – 14 – – – –
Cantat-Gaudin & Anders 2020 5.54 – – – – – – –
Dias et al. 2019 4.34 1.36 – 23 -0.642 – – –
Bossini et al. 2019 5.89 1.89 – 14 0.000 – – –
Cantat-Gaudin et al. 2018 5.54 – – – – – – –
Loktin & Popova 2017 4.64 1.91 – 9 – – – –
Kharchenko et al. 2016 4.67 1.87 – 6 – – – –
Kharchenko et al. 2013 4.67 1.87 – 6 – – – –
Piskunov et al. 2008 4.66 1.92 – 21 – – – –
van den Bergh 2006 4.73 1.92 – 9 – – – –
Kharchenko et al. 2005 4.66 1.92 – 21 – – – –
Dias et al. 2002 4.73 1.92 – 9 – – – –
Dambis 1999 3.89 2.00 – 3 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1429 9.6 119.42 -28.54 0.21 -2.31 2.89 76.8 0.41

💡 Note: The % column shows the percentage of members that Ruprecht 44 shares with each listed object.

Visualization

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