Teutsch 40

(MWSC 3129; DSH J1929.2+2318)

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0.14 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.29
Clit
1.0
Cdup
Core radius and density 7.7 [pc], 0.08 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

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Teutsch 40 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.55 kpc) differs significantly from the median photometric distance (~3.15 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 292.311 23.291 0.22 -2.423 -4.051 –
Just et al. 2023 292.337 23.298 – – – –
Bica et al. 2019 292.317 23.302 – – – –
Dias et al. 2018 – – – -1.54 -4.87 –
Loktin & Popova 2017 292.32 23.3 – -1.458 -4.703 –
Sampedro et al. 2017 292.317 23.311 – -4.33 0.6 –
Kharchenko et al. 2016 292.337 23.298 – – – –
Dias et al. 2014 292.317 23.311 – -3.83 -0.12 –
Kharchenko et al. 2013 292.342 23.3 – -2.31 -3.39 –
Bukowiecki et al. 2011 292.308 23.306 – – – –
Kronberger et al. 2006 292.32 23.305 – – – –
Dias et al. 2002 292.317 23.311 – -3.83 -0.12 –

💡 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– 3.15 3.02 – 1303 – 448 – –
Just et al. 2023 – – – 1303 – 448 – –
Loktin & Popova 2017 3.62 2.23 – 933 – – – –
Kharchenko et al. 2016 3.15 3.02 – 1303 – – – –
Kharchenko et al. 2013 3.15 3.02 – 1303 – – – –
Dias et al. 2002 2.98 3.03 – 794 – – – –

Visualization

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