NGC 2394

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0.12 UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.16
Clit
1.0
Cdup
Core radius and density 2.7 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.25 Low quality
  • Clit 0.16 Rarely studied
  • Cdup 1.0 Unique

Overview

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NGC 2394 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~3.96 kpc) differs significantly from the median photometric distance (~0.94 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.

Cantat-Gaudin & Anders (2020)
Flagged as non-existent in the Revised NGC. Sparse CMD-based estimates exist, but it is considered an asterism in recent compilations. More details in Appendix A of the article.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 112.145 7.101 0.253 -1.039 -0.577 –
Dias et al. 2018 – – – -2.61 -0.17 –
Loktin & Popova 2017 112.14 7.087 – -6.02 -4.569 –
Sampedro et al. 2017 112.15 7.087 – – – –
Dias et al. 2014 112.15 7.087 – -0.27 -0.83 –
Bukowiecki et al. 2011 112.158 7.161 – – – –
Dias et al. 2002 112.15 7.087 – -0.27 -0.83 –

💡 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– 0.94 0.41 – 891 – 88 – –
Loktin & Popova 2017 2.48 0.13 – 832 – – – –
Bukowiecki et al. 2012 – – – – – 88 – –
Bukowiecki et al. 2011 0.94(1) 0.41 – 891 – – – –
Dias et al. 2002 0.94 0.41 – 891 – – – –

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

Visualization

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