NGC 2239

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0.43 UTI
0.47
CN
0.52
Cdens
0.75
CC3
0.19
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 2.6 [pc-2]
  • CN 0.47 Poorly populated
  • Cdens 0.52 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

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NGC 2239 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by high 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 6 years.

(*): The parallax distance estimate (~1.49 kpc) differs significantly from the median photometric distance (~3.51 kpc).

Note: This object shares a moderate percentage of members 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– 97.756 4.939 0.673 -1.834 0.029 24.063
SΓ‘nchez et al. 2020 97.737 4.969 – -1.614 -0.338 –
Dias et al. 2018 – – – -3.0 -1.16 –
Loktin & Popova 2017 97.74 4.97 – -0.6 -2.18 –
Sampedro et al. 2017 97.737 4.969 – 0.01 -0.78 –
Dias et al. 2014 97.737 4.969 – -0.6 -2.18 –
Dias et al. 2002 97.737 4.969 – -0.6 -2.18 –
Lynga 1987 97.727 4.953 – – – –
Sulentic et al. 1973 97.733 4.948 – – – –

πŸ’‘ 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– 3.51 3.02 – 304 – – – –
Loktin & Popova 2017 3.12 2.57 – 603 – – – –
Dias et al. 2002 3.90 3.47 – 5 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 2244 31.9 98.01 4.91 0.65 -1.71 0.23 27.15 0.93

πŸ’‘ Note: The % column shows the percentage of members that NGC 2239 shares with each listed object.

Visualization

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