Teutsch 126

(MWSC 3599; DSH J2213.7+5543)

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0.95 UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.76 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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Teutsch 126 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good 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 – 333.456 55.72 0.444 -1.853 -2.245 -61.37
Li et al. 2025 333.455 55.712 0.437 -1.82 -2.23 –
Almeida et al. 2025 333.462 55.705 – – – –
Hunt & Reffert 2024 333.477 55.731 0.433 -1.869 -2.257 -69.516
Cavallo et al. 2024 333.449 55.718 0.442 – – –
Hunt & Reffert 2023 333.477 55.731 0.433 -1.869 -2.257 -69.516
Almeida et al. 2023 333.454 55.699 – – – –
Just et al. 2023 333.433 55.75 – – – –
Dias et al. 2021 333.462 55.705 0.436 -1.799 -2.231 –
Cantat-Gaudin et al. 2020 333.455 55.712 0.437 -1.82 -2.23 –
Cantat-Gaudin & Anders 2020 333.455 55.712 0.437 -1.82 -2.23 –
Soubiran et al. 2018 333.455 55.712 – – – -33.73
Bica et al. 2019 333.438 55.731 – – – –
Cantat-Gaudin et al. 2018 333.455 55.712 0.437 -1.82 -2.23 –
Loktin & Popova 2017 333.435 55.721 – -0.983 -2.898 –
Kharchenko et al. 2016 333.433 55.75 – – – –
Dias et al. 2014 333.442 55.72 – -1.52 -2.41 –
Kharchenko et al. 2013 333.439 55.753 – -0.08 -3.07 –
Kharchenko et al. 2012 333.439 55.753 – -0.08 -3.07 –
Kronberger et al. 2006 333.446 55.731 – – – –
Dias et al. 2002 333.442 55.72 – -1.52 -2.41 –

💡 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] Bfr BSS
Li et al. 2025 1.78 0.83 – 444 -0.052 – – –
Almeida et al. 2025 1.92 1.35 – 109 – 317 – –
Hunt & Reffert 2024 – – – – – 538* – –
Cavallo et al. 2024 2.42 1.50 – 83 0.660 – – –
Hunt & Reffert 2023 2.10 1.35 1.94 103 – – – –
Almeida et al. 2023 1.92 1.36 – 99 0.051 483* 0.53 –
Just et al. 2023 – – – 631 – 30 – –
Dias et al. 2021 1.92 1.35 – 109 0.097 – – –
Cantat-Gaudin et al. 2020 2.23 1.13 – 49 – – – –
Cantat-Gaudin & Anders 2020 2.15 – – – – – – –
Soubiran et al. 2018 2.15 – – – – – – –
Cantat-Gaudin et al. 2018 2.15 – – – – – – –
Loktin & Popova 2017 2.22 1.60 – 4 – – – –
Kharchenko et al. 2016 1.82 1.94 – 631 – – – –
Kharchenko et al. 2013 1.82 1.94 – 631 – – – –
Kharchenko et al. 2012 1.82 1.94 – 631 – – – –
Dias et al. 2002 1.74 0.68 – 398 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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