Czernik 11

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0.15 UTI
0.0
CN
0.09
Cdens
0.12
CC3
0.26
Clit
1.0
Cdup
Core radius and density 1.4 [pc], 0.5 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.26 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Czernik 11 is a sparse, 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 an intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~3.30 kpc) differs significantly from the median photometric distance (~1.50 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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 39.189 59.637 0.303 -0.606 -0.092 -50.779
Dib et al. 2018 39.144 59.634 – – – –
Loktin & Popova 2017 39.135 59.632 – -1.123 -4.417 –
Sampedro et al. 2017 39.146 59.633 – – – –
Joshi et al. 2016 39.144 59.634 – – – –
Tadross 2014 39.146 59.633 – – – –
Dias et al. 2014 39.146 59.633 – -0.08 -0.53 –
Bukowiecki et al. 2011 39.163 59.667 – – – –
Dias et al. 2002 39.146 59.633 – -0.08 -0.53 –
Lynga 1987 38.953 59.633 – – – –

💡 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– 1.5 3.15 – 348 – 173 – –
Dib et al. 2018 1.50 – – 359 – – – –
Loktin & Popova 2017 2.35 4.61 – 100 – – – –
Joshi et al. 2016 1.50 3.15 – 359 – – – –
Tadross 2014 1.21 3.15 – 350 – – – –
Bukowiecki et al. 2012 – – – – – 173 – –
Bukowiecki et al. 2011 2.13(1) 3.12 – 32 – – – –
Dias et al. 2002 1.21 3.15 – 347 – – – –

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

Visualization

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