FoF 2172

(LP 2172)

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0.43 UTI
0.39
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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FoF 2172 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close High extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 282.464 -0.323 0.476 -0.396 -1.924 -163.47
Almeida et al. 2025 282.482 -0.323 – – – –
Dias et al. 2021 282.482 -0.323 0.48 -0.433 -1.838 9.956

💡 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 1.92 4.01 – 43 – 375 – –
Dias et al. 2021 1.92 4.01 – 43 0.137 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2352 97.4 282.46 -0.33 0.48 -0.42 -1.98 -31.63 0.07
OC 0064 94.9 282.46 -0.33 0.49 -0.4 -1.96 -31.63 0.2

💡 Note: The % column shows the percentage of members that FoF 2172 shares with each listed object.

Visualization

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