FoF 1620

(LP 1620)

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0.56 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.78 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 1620 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 very massive, near-solar metallicity, old cluster (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.

Distant High extinction Very massive Near-solar metallicity Old

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 – 252.993 -44.229 0.342 -1.318 -1.169 -64.5
Almeida et al. 2025 252.986 -44.233 – – – –
He et al. 2023 252.99 -44.233 0.345 -1.321 -1.172 -64.5
Dias et al. 2021 252.986 -44.233 0.328 -1.342 -1.113 –

💡 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 3.82 3.18 – 2460 – 5717 – –
He et al. 2023 2.29 4.90 – 794 – – – –
Dias et al. 2021 3.82 3.18 – 2460 0.234 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2833 100.0 252.99 -44.23 0.35 -1.32 -1.18 -63.64 0.19

💡 Note: The % column shows the percentage of members that FoF 1620 shares with each listed object.

Visualization

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