FoF 2221

(LP 2221)

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0.41 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.74
Cdup
Radius (P>50% members) 8.8 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.74 Likely unique

Overview

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FoF 2221 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Close Moderate extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 129.428 -40.234 1.058 -5.616 3.77 21.566
Almeida et al. 2025 129.44 -40.028 – – – –
Dias et al. 2021 129.44 -40.028 1.025 -5.564 3.846 41.227

💡 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] Bfr BSS
Almeida et al. 2025 0.93 1.23 – 9 – 512 – –
Dias et al. 2021 0.93 1.23 – 9 -0.059 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0467 62.1 129.4 -40.29 1.06 -5.67 3.69 19.99 0.09
Pismis 5 25.8 129.41 -39.62 1.05 -5.48 4.26 19.64 0.92
CWNU 1239 2.2 129.85 -40.54 1.06 -5.38 3.47 -15.31 0.13

💡 Note: The % column shows the percentage of members that FoF 2221 shares with each listed object.

Visualization

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