FoF 1175

(LP 1175)

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0.48 UTI
0.66
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.66 Moderately 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 1175 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

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

Distant High extinction Near-solar metallicity Very 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 – 223.892 -60.518 0.304 -5.178 -3.33 31.705
Almeida et al. 2025 223.901 -60.524 – – – –
Dias et al. 2021 223.901 -60.524 0.289 -5.189 -3.356 –

💡 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 3.20 3.50 – 6 – 685 – –
Dias et al. 2021 3.20 3.50 – 6 0.165 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0619 30.1 223.9 -60.52 0.31 -5.18 -3.34 47.79 0.0

💡 Note: The % column shows the percentage of members that FoF 1175 shares with each listed object.

Visualization

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