Teutsch 132

(MWSC 477)

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0.62 UTI
0.33
CN
1.0
Cdens
0.25
CC3
0.75
Clit
1.0
Cdup
C3 classification CC
Number of members (P>50%) 33
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
Teutsch 132 is a poorly populated, very dense object of low 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, very young cluster (see Parameters). It is well-studied in the literature.
Distant Moderate extinction Near-solar metallicity Very young

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

Data
πŸ” Search references for Teutsch 132 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 77.507 38.817 0.264 0.196 -1.553 –
Almeida et al. 2025 77.514 38.816 – – – –
He et al. 2023 77.515 38.817 0.278 0.045 -1.553 13.86
Almeida et al. 2023 77.514 38.816 – – – –
Just et al. 2023 77.473 38.815 – – – –
Dias et al. 2021 77.514 38.816 0.223 0.326 -1.536 –
SΓ‘nchez et al. 2020 77.504 38.825 – 0.304 -1.619 –
Loktin & Popova 2017 77.505 38.825 – -1.206 -0.673 –
Kharchenko et al. 2016 77.473 38.815 – – – –
Dias et al. 2014 77.504 38.825 – -1.92 -2.24 –
Kharchenko et al. 2013 77.482 38.815 – -4.39 -0.22 –
Kharchenko et al. 2012 77.482 38.815 – -4.39 -0.22 –
Kronberger et al. 2006 77.503 38.821 – – – –
Dias et al. 2002 77.504 38.825 – -1.92 -2.24 –

πŸ’‘ 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
Almeida et al. 2025 3.47 2.22 – 10 – 499 – –
He et al. 2023 2.95 2.20 – 50 – – – –
Almeida et al. 2023 3.12 2.21 – 17 -0.212 309* 0.61 –
Just et al. 2023 – – – 8 – 195 – –
Dias et al. 2021 3.47 2.22 – 10 -0.160 – – –
Loktin & Popova 2017 3.69 1.39 – 692 – – – –
Kharchenko et al. 2016 4.00 2.48 – 8 – – – –
Kharchenko et al. 2013 4.00 2.48 – 8 – – – –
Kharchenko et al. 2012 4.00 2.48 – 8 – – – –
Dias et al. 2002 5.37 2.33 – 5 – – – –

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

Visualization
ℹ️
Teutsch 132 UCC
Galactocentric position diagram