NGC 2360

(Melotte 64; Collinder 134; MWSC 1165; OCL 589; FSR 1225; FoF 2083)

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1.0 UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 86.2 [N/pc2]
  • CN 1.0 Very 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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NGC 2360 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

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

Malhotra et al. (2026)
Lowest/Highest stellar mass in the catalogue with a mass-ratio estimate: 0.49/1.81 Msun

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Ahumada & Lapasset (2007)
Stars 51 and 100 are cited as blue stragglers in (1968ApJ...152...83E) and (1994AJ....108.1828M). The last reference also considers stars 1, 69, and 82 (WEBDA numbers) as stragglers. Adopted cluster centre: star 46 (1968ApJ...152...83E).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 109.44 -15.631 0.917 0.376 5.628 27.693
Malhotra et al. 2026 109.441 -15.639 – – – –
Li et al. 2025 109.443 -15.631 0.902 0.383 5.603 –
Hu & Soubiran 2025 109.436 -15.633 – – – –
Wei et al. 2025 109.44 -15.635 0.918 0.382 5.63 –
Almeida et al. 2025 109.44 -15.63 – – – –
Hunt & Reffert 2024 109.441 -15.644 0.917 0.385 5.629 27.246
Cavallo et al. 2024 109.436 -15.633 0.916 – – –
Hunt & Reffert 2023 109.441 -15.644 0.917 0.385 5.629 27.246
Almeida et al. 2023 109.438 -15.628 – – – –
Angelo et al. 2023 109.463 -15.629 – 0.39 5.63 –
Cordoni et al. 2023 109.44 -15.63 0.9 0.389 5.608 –
Just et al. 2023 109.419 -15.638 – – – –
He et al. 2022 109.435 -15.635 0.918 0.389 5.634 –
Tarricq et al. 2022 109.44 -15.639 0.924 0.376 5.63 –
Jadhav & Subramaniam 2021 109.443 -15.631 – – – –
Jaehnig et al. 2021 109.444 -15.637 0.931 0.363 5.591 –
Rain et al. 2021 109.443 -15.631 0.902 0.383 5.603 –
Dias et al. 2021 109.44 -15.63 0.9 0.389 5.608 28.386
Cantat-Gaudin et al. 2020 109.443 -15.631 0.902 0.383 5.603 –
Cantat-Gaudin & Anders 2020 109.443 -15.631 0.902 0.383 5.603 –
Liu & Pang 2019 109.442 -15.626 0.903 0.393 5.595 –
Soubiran et al. 2018 109.443 -15.631 – – – 28.3
Bica et al. 2019 109.455 -15.654 – – – –
Cantat-Gaudin et al. 2018 109.443 -15.631 0.902 0.383 5.603 –
Loktin & Popova 2017 109.425 -15.641 – -1.792 6.032 25.5
Kharchenko et al. 2016 109.419 -15.638 – – – –
Dias et al. 2014 109.429 -15.642 – -1.51 5.27 –
Kharchenko et al. 2013 109.425 -15.64 – -2.3 6.6 25.5
Gozha et al. 2012 109.429 -15.642 – – – –
Bukowiecki et al. 2011 109.433 -15.631 – – – –
Piskunov et al. 2008 109.422 -15.637 – – – –
Kharchenko et al. 2007 109.42 -15.64 – 0.25 – 25.47
Piskunov et al. 2007 109.422 -15.637 – – – –
Ahumada & Lapasset 2007 109.425 -15.65 – – – –
van den Bergh 2006 109.425 -15.633 – – – –
Kharchenko et al. 2005 109.42 -15.64 – -2.62 4.89 25.47
Kharchenko et al. 2003 109.44 -15.63 – -2.6 4.82 –
Chen et al. 2003 109.436 -15.63 – 3.51 8.07 27.2
Dias et al. 2002 109.429 -15.642 – -3.51 8.07 27.28
Lynga 1987 109.431 -15.633 – – – –
Sulentic et al. 1973 109.409 -15.646 – – – –

💡 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– 1.1 0.35 0.34 1000 -0.083 1316 0.41 0
Malhotra et al. 2026 1.08 0.31 – 1074 -0.030 – – –
Li et al. 2025 1.02 0.41 – 1361 -0.175 – – –
Hu & Soubiran 2025 – – – – -0.210(5) – – –
Wei et al. 2025 1.11 0.49 – 1410 -0.250 1589 0.30 –
Almeida et al. 2025 1.05 0.41 – 1268 – 1671 – –
Hunt & Reffert 2024 – – – – – 2771(1) – –
Cavallo et al. 2024 1.09 0.35 – 1175 0.290 – – –
Hunt & Reffert 2023 1.01 0.12 0.34 1452 – – – –
Almeida et al. 2023 1.04 0.40 – 1276 -0.083 1327(1) 0.41 –
Angelo et al. 2023 0.95 0.38 – 1413 -0.220 8(1) – –
Cordoni et al. 2023 1.05 0.41 – 1268 -0.045 1656 0.41 0(1)
Just et al. 2023 – – – 447 – 543 – –
He et al. 2022 – 0.55 – 891 – – – –
Tarricq et al. 2022 1.09 – – 1000 – – – –
Jadhav & Subramaniam 2021 1.12 0.39 – 1023 – 3104 – 0(1)
Jaehnig et al. 2021 1.07(1) – – – – – – –
Rain et al. 2021 1.07 0.03 – 631 – – – 1
Dias et al. 2021 1.05 0.41 – 1268 -0.045 – – –
Cantat-Gaudin et al. 2020 1.12 0.39 – 1023 – – – –
Kounkel et al. 2020 1.07 0.62 – 891 – – – –
Cantat-Gaudin & Anders 2020 1.07 – – – – – – –
Liu & Pang 2019 – – – 1410 -0.250 – – –
Soubiran et al. 2018 1.07 – – – – – – –
Cantat-Gaudin et al. 2018 1.07 – – – – – – –
Loktin & Popova 2017 1.89 0.35 – 592 – – – –
Kharchenko et al. 2016 1.56 1.31 – 447 – – – –
Kharchenko et al. 2013 1.56 1.31 – 447 -0.030 – – –
Bukowiecki et al. 2012 – – – – – 1305 – –
Gozha et al. 2012 1.89 – – 561 -0.030 1000 – –
Bukowiecki et al. 2011 1.17(1) 0.00 – 1413 – – – –
Piskunov et al. 2008 1.89 0.35 – 389 – 955(1) – –
Piskunov et al. 2007 1.89 0.35 – 389 – 255 – –
Ahumada & Lapasset 2007 – 0.35 – 562 – – – 4
van den Bergh 2006 1.89 0.35 – 562 – – – –
Kharchenko et al. 2005 1.89 0.35 – 389 – – – –
Kharchenko et al. 2003 1.89 0.35 – – – – – –
Chen et al. 2003 1.89 0.35 – 560 -0.150(1) – – –
Dias et al. 2002 1.12 0.03 – 631 -0.030 – – –
Lynga 1987 1.63 0.19 – 1288 -0.130 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0391 3.6 109.45 -15.63 0.98 0.41 5.55 27.51 0.0
HSC 1815 1.8 109.44 -15.78 1.1 0.49 5.45 – 0.02

💡 Note: The % column shows the percentage of members that NGC 2360 shares with each listed object.

Visualization

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