NGC 6938

(MWSC 3372)

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0.10 UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.19
Clit
1.0
Cdup
Core radius and density 6.2 [pc], 0.06 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 6938 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.68 kpc) differs significantly from the median photometric distance (~1.68 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.

Dias et al. (2022)
Likely not a real open cluster.

Bica et al. (2019)
Original NGC and IC catalogues at Vizier: NGC 2000.0, Sky Publishing, ed. Sinnott 1988 (1997yCat.7118....0S).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 308.696 22.175 0.272 -2.793 -4.651 –
Bica et al. 2019 308.672 22.216 – – – –
Loktin & Popova 2017 308.67 22.214 – -0.655 -0.408 –
Sampedro et al. 2017 308.675 22.215 – 0.59 -3.05 –
Tadross 2014 308.675 22.215 – – – –
Dias et al. 2014 308.675 22.215 – 0.63 -3.64 –
Bukowiecki et al. 2011 308.65 22.246 – – – –
Dias et al. 2002 308.675 22.215 – 0.55 -3.55 –

💡 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– 1.68 0.41 – 1294 – 95 – –
Loktin & Popova 2017 2.27 0.17 – 1622 – – – –
Tadross 2014 1.25 0.41 – 1300 – – – –
Bukowiecki et al. 2012 – – – – – 95 – –
Bukowiecki et al. 2011 2.11(1) 1.77 – 224 – – – –
Dias et al. 2002 1.25 0.41 – 1288 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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