Teutsch 103

(SAI 107; MWSC 1674; DSH J0928.5-4636; FSR 1472)

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0.82 UTI
0.6
CN
1.0
Cdens
0.5
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.6 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Teutsch 103 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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 parameter (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: intermediate fit. Silver sample.

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 – 142.148 -46.605 0.361 -4.991 3.341 18.083
Li et al. 2025 142.145 -46.607 0.356 -5.055 3.342 –
Almeida et al. 2025 142.151 -46.61 – – – –
Hunt & Reffert 2024 142.144 -46.605 0.351 -4.96 3.326 18.045
Cavallo et al. 2024 142.165 -46.6 0.354 – – –
Hunt & Reffert 2023 142.144 -46.605 0.351 -4.96 3.326 18.045
Almeida et al. 2023 142.157 -46.608 – – – –
Just et al. 2023 142.149 -46.597 – – – –
Dias et al. 2021 142.151 -46.61 0.38 -5.03 3.284 –
Cantat-Gaudin et al. 2020 142.145 -46.607 0.356 -5.055 3.342 –
Cantat-Gaudin & Anders 2020 142.145 -46.607 0.356 -5.055 3.342 –
Soubiran et al. 2018 142.145 -46.607 – – – 18.46
Bica et al. 2019 142.143 -46.604 – – – –
Cantat-Gaudin et al. 2018 142.145 -46.607 0.356 -5.055 3.342 –
Kharchenko et al. 2016 142.149 -46.597 – – – –
Dias et al. 2014 142.15 -46.6 – -4.74 2.19 –
Kharchenko et al. 2013 142.155 -46.6 – -8.48 4.69 –
Glushkova et al. 2010 142.149 -46.6 – – – –
Kronberger et al. 2006 142.147 -46.608 – – – –
Dias et al. 2002 142.15 -46.6 – -4.74 2.19 –

💡 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 3.91 2.94 – 1479 -0.031 – – –
Almeida et al. 2025 2.29 2.66 – 533 – 243 – –
Hunt & Reffert 2024 – – – – – 218* – –
Cavallo et al. 2024 2.67 3.03 – 316 0.090 – – –
Hunt & Reffert 2023 2.60 3.03 0.90 216 – – – –
Almeida et al. 2023 2.44 2.75 – 459 -0.027 235* 0.48 –
Just et al. 2023 – – – 944 – 184 – –
Dias et al. 2021 2.29 2.66 – 533 -0.029 – – –
Cantat-Gaudin et al. 2020 2.81 2.36 – 363 – – – –
Cantat-Gaudin & Anders 2020 2.60 – – – – – – –
Soubiran et al. 2018 2.60 – – – – – – –
Cantat-Gaudin et al. 2018 2.60 – – – – – – –
Kharchenko et al. 2016 2.66 2.90 – 944 – – – –
Kharchenko et al. 2013 2.66 2.90 – 944 – – – –
Glushkova et al. 2010 2.79 1.92 – 562 – – – –
Dias et al. 2002 2.79 1.92 – 562 – – – –

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

Visualization

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