Turner 1

(MWSC 3184)

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0.21 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Turner 1 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 moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.92 kpc) differs significantly from the median photometric distance (~2.79 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.

Relatively close Moderate extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 297.118 27.281 0.255 -3.795 -6.529 -67.629
Just et al. 2023 297.107 27.293 – – – –
Loktin & Popova 2017 297.12 27.298 – -3.802 -2.805 0.5
Kharchenko et al. 2016 297.107 27.293 – – – –
Dias et al. 2014 297.104 27.293 – -3.48 -3.81 0.5
Kharchenko et al. 2013 297.112 27.295 – -4.39 -3.22 –
van den Bergh 2006 297.267 27.298 – – – –
Dias et al. 2002 297.104 27.293 – -3.48 -3.81 0.5

💡 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
Just et al. 2023 – – – 550 – 350 – –
Loktin & Popova 2017 3.98 1.58 – 1023 – – – –
Kharchenko et al. 2016 2.79 1.68 – 550 – – – –
Kharchenko et al. 2013 2.79 1.68 – 550 – – – –
van den Bergh 2006 1.68 1.49 – 29 – – – –
Dias et al. 2002 1.68 1.48 – 29 – – – –

Visualization

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