FoF 1641

(LP 1641)

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0.50 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 13.7 [N/pc2]
  • CN 0.75 Rich
  • 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 1641 is a rich, 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 massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.

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

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 99999– 277.912 -10.166 0.315 -1.172 -3.306 34.01
Almeida et al. 2025 277.916 -10.175 – – – –
He et al. 2023 277.916 -10.168 0.306 -1.163 -3.335 33.66
Dias et al. 2021 277.916 -10.175 0.32 -1.209 -3.254 33.852

💡 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– 3.4 4.12 – 5 0.152 1568 – –
Almeida et al. 2025 3.40 4.12 – 5 – 1568 – –
He et al. 2023 2.69 5.35 – 50 – – – –
Dias et al. 2021 3.40 4.12 – 5 0.152 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 230 85.7 277.91 -10.17 0.31 -1.17 -3.33 33.58 0.09

💡 Note: The % column shows the percentage of members that FoF 1641 shares with each listed object.

Visualization

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