Czernik 4

(MWSC 126)

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0.28 UTI
0.25
CN
0.12
Cdens
0.12
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.12 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Czernik 4 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.16 kpc) differs significantly from the median photometric distance (~1.67 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 23.886 61.493 0.316 -2.289 -0.352 -49.201
Just et al. 2023 23.891 61.461 – – – –
Loktin & Popova 2017 23.895 61.476 – 1.987 -2.909 -11.4
Kharchenko et al. 2016 23.891 61.461 – – – –
Kharchenko et al. 2013 23.902 61.463 – 1.84 -1.84 -11.4
Kharchenko et al. 2012 23.902 61.463 – 0.13 -3.9 –
Bukowiecki et al. 2011 23.913 61.46 – – – –
Dias et al. 2002 23.9 61.476 – 0.13 -3.9 -11.4

💡 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– 1.665 3.1 – 52 – 202 – –
Just et al. 2023 – – – 52 – 16 – –
Loktin & Popova 2017 2.18 1.22 – 100 – – – –
Kharchenko et al. 2016 1.63 3.10 – 52 – – – –
Kharchenko et al. 2013 1.63 3.10 – 52 – – – –
Bukowiecki et al. 2012 – – – – – 389 – –
Kharchenko et al. 2012 1.70 3.10 – 132 – – – –
Bukowiecki et al. 2011 2.96(1) 2.88 – 32 – – – –
Dias et al. 2002 1.63 3.29 – 100 – – – –

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

Visualization

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