FoF 1625

(LP 1625)

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0.57 UTI
0.84
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.84 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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FoF 1625 is a rich, very dense object of very 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, intermediate-age 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 significant percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Intermediate age

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 – 269.495 -23.285 0.296 -0.087 -1.643 -11.446
Almeida et al. 2025 269.491 -23.284 – – – –
He et al. 2023 269.493 -23.285 0.289 -0.083 -1.676 -11.85
Dias et al. 2021 269.491 -23.284 0.312 -0.131 -1.583 22.824

💡 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 3.11 3.88 – 802 – 4771 – –
He et al. 2023 2.75 5.90 – 200 – – – –
Dias et al. 2021 3.11 3.88 – 802 0.333 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 92 72.7 269.49 -23.29 0.28 -0.07 -1.67 -11.29 0.03

💡 Note: The % column shows the percentage of members that FoF 1625 shares with each listed object.

Visualization

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