FoF 733

(FoF 0733; LP 0733)

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0.20 UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.4
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.4 Possibly duplicate

Overview

â„šī¸
FoF 733 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 111.068 -20.234 0.322 -2.636 3.086 66.236
Almeida et al. 2025 111.071 -20.245 – – – –
Almeida et al. 2023 111.073 -20.246 – – – –
Dias et al. 2021 111.071 -20.245 0.305 -2.433 3.018 56.303

💡 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 2.71 1.04 – 49 – 921 – –
Almeida et al. 2023 2.61 1.11 – 33 -0.149 936* 0.57 –
Dias et al. 2021 2.71 1.04 – 49 -0.112 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PHOC 16 60.3 111.05 -20.21 0.33 -2.73 3.12 66.24 0.6
CWWDL 630 22.2 111.07 -20.25 0.32 -2.44 3.07 – 0.0

💡 Note: The % column shows the percentage of members that FoF 733 shares with each listed object.

Visualization

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