FoF 2312

(LP 2312)

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0.55 UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.5 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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FoF 2312 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 223.136 -61.495 0.93 -2.247 -1.856 12.656
Almeida et al. 2025 223.12 -61.506 – – – –
Almeida et al. 2023 223.139 -61.509 – – – –
He et al. 2022 223.125 -61.487 0.931 -2.271 -1.878 –
Dias et al. 2021 223.12 -61.506 0.923 -2.223 -1.848 –

💡 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 1.06 1.85 – 52 – 152 – –
Almeida et al. 2023 1.02 1.75 – 145 0.042 198* 0.75 –
He et al. 2022 – 2.10 – 50 – – – –
Dias et al. 2021 1.06 1.85 – 52 0.074 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 2325 100.0 223.14 -61.5 0.93 -2.24 -1.86 0.63 0.13
OC 0616 59.3 223.14 -61.47 0.93 -2.27 -1.86 23.94 0.0

💡 Note: The % column shows the percentage of members that FoF 2312 shares with each listed object.

Visualization

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