NGC 1220

(Collinder 37; MWSC 261; OCL 380)

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0.87 UTI
0.62
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 32.3 [N/pc2]
  • CN 0.62 Moderately populated
  • 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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NGC 1220 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

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: 0.94 (50th percentile).

Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=7.957, Av=2.162, [Fe/H]=0.00 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 47.921 53.345 0.327 0.193 -0.805 -39.756
Almeida et al. 2025 47.92 53.346 – – – –
Hunt & Reffert 2024 47.923 53.35 0.351 0.187 -0.814 -58.92
Cavallo et al. 2024 47.922 53.346 0.341 – – –
Hunt & Reffert 2023 47.923 53.35 0.351 0.187 -0.814 -58.92
Almeida et al. 2023 47.92 53.346 – – – –
Just et al. 2023 47.91 53.345 – – – –
Jaehnig et al. 2021 47.919 53.347 0.342 0.202 -0.753 –
Rain et al. 2021 47.92 53.344 0.297 0.187 -0.717 –
Dias et al. 2021 47.92 53.346 0.305 0.181 -0.72 –
Cantat-Gaudin et al. 2020 47.92 53.344 0.297 0.187 -0.717 –
Zhong et al. 2020 47.92 53.344 – 0.187 -0.717 -53.838
Cantat-Gaudin & Anders 2020 47.92 53.344 0.297 0.187 -0.717 –
Bossini et al. 2019 47.92 53.344 – – – –
Soubiran et al. 2018 47.92 53.344 – – – -15.53
Bica et al. 2019 47.91 53.351 – – – –
Cantat-Gaudin et al. 2018 47.92 53.344 0.297 0.187 -0.717 –
Loktin & Popova 2017 47.91 53.345 – -0.173 3.251 –
Kharchenko et al. 2016 47.91 53.345 – – – –
Dias et al. 2014 47.917 53.345 – -0.13 -0.5 –
Kharchenko et al. 2013 47.922 53.347 – 0.3 0.4 –
Kharchenko et al. 2012 47.922 53.347 – 0.3 0.4 –
Bukowiecki et al. 2011 47.925 53.341 – – – –
Ahumada & Lapasset 2007 47.925 53.35 – – – –
van den Bergh 2006 47.925 53.333 – – – –
Dias et al. 2002 47.917 53.345 – -0.13 -0.5 –
Lynga 1987 47.93 53.332 – – – –
Sulentic et al. 1973 47.908 53.344 – – – –

💡 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– 2.91 2.37 1.56 85 0.000 303 0.54 0
Almeida et al. 2025 2.40 2.45 – 24 – 411 – –
Hunt & Reffert 2024 – – – – – 900(1) – –
Cavallo et al. 2024 2.95 2.47 – 85 0.370 – – –
Hunt & Reffert 2023 2.70 2.41 1.56 114 – – – –
Almeida et al. 2023 2.49 2.48 – 36 -0.113 255(1) 0.54 –
Just et al. 2023 – – – 158 – 85 – –
Jaehnig et al. 2021 2.91(1) – – – – – – –
Rain et al. 2021 3.07 2.18 – 89 – – – 0
Dias et al. 2021 2.40 2.45 – 24 -0.140 – – –
Cantat-Gaudin et al. 2020 3.06 2.33 – 49 – – – –
Kounkel et al. 2020 3.22 2.51 – 117 – – – –
Zhong et al. 2020 3.07(1) 2.37 – 8200 0.000 – – –
Cantat-Gaudin & Anders 2020 3.07 – – – – – – –
Bossini et al. 2019 3.19 2.16 – 91 0.000 – – –
Soubiran et al. 2018 3.07 – – – – – – –
Cantat-Gaudin et al. 2018 3.07 – – – – – – –
Loktin & Popova 2017 3.17 2.10 – 73 – – – –
Kharchenko et al. 2016 2.10 2.37 – 158 – – – –
Kharchenko et al. 2013 2.10 2.37 – 158 – – – –
Bukowiecki et al. 2012 – – – – – 303 – –
Kharchenko et al. 2012 2.10 2.37 – 158 – – – –
Bukowiecki et al. 2011 2.45(1) 1.96 – 79 – – – –
Ahumada & Lapasset 2007 – 2.21 – 60 – – – 0
van den Bergh 2006 1.80 2.21 – 60 – – – –
Dias et al. 2002 1.80 2.21 – 60 – – – –

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

Visualization

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