NGC 2678

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0.02 UTI
0.0
CN
0.13
Cdens
0.75
CC3
0.13
Clit
0.08
Cdup
Core radius and density 2.2 [pc], 0.6 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.75 High quality
  • Clit 0.13 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

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NGC 2678 is a sparse, very loose object of high C3 quality. Its parallax locates it at a close distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 132.579 11.358 1.049 -10.918 -2.821 35.483
Donor et al. 2020 132.508 11.338 – -11.01 -3.08 34.1
Sampedro et al. 2017 132.508 11.338 – -2.56 -5.2 –
Tadross 2014 132.508 11.338 – – – –
Dias et al. 2014 132.508 11.338 – -4.32 -3.55 33.67
Dias et al. 2002 132.508 11.338 – -4.14 -3.39 33.67

💡 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– 0.9 0.09 – 2296 0.000 – – –
Spina et al. 2022 – – – – 0.000 – – –
Donor et al. 2020 – – – – 0.000 – – –
Tadross 2014 0.90 0.09 – 2300 – – – –
Dias et al. 2002 0.90 0.09 – 2291 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 2682 92.0 132.85 11.82 1.15 -10.97 -2.91 33.91 1.0
CWWDL 14090 36.0 132.84 11.82 1.15 -10.98 -2.91 33.79 0.0
Chupina 3 4.0 132.85 11.41 1.15 -11.04 -2.83 34.39 0.0

💡 Note: The % column shows the percentage of members that NGC 2678 shares with each listed object.

Visualization

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