FoF 1174

(LP 1174)

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0.06 UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FoF 1174 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Massive Near-solar metallicity Very young

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 219.482 -61.115 0.284 -5.276 -2.934 -70.429
Almeida et al. 2025 219.366 -61.076 – – – –
Dias et al. 2021 219.366 -61.076 0.273 -5.3 -2.936 -61.452

💡 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 3.56 2.74 – 8 – 1338 – –
Dias et al. 2021 3.56 2.74 – 8 0.049 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0613 12.0 219.79 -61.08 0.18 -5.3 -3.07 51.07 0.42

💡 Note: The % column shows the percentage of members that FoF 1174 shares with each listed object.

Visualization

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