FoF 1994

(LP 1994)

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C3
N_50
r_50
AA 208 5.6
Summary

FoF 1994 is a rich, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is moderately studied in the literature.

This object shares a large percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Liu & Pang (2019) 190.974 -58.089 0.5 -2.185 -1.25
Cantat-Gaudin et al. (2020) 191.005 -58.096 0.501 -2.174 -1.294
Dias et al. (2021) 190.997 -58.093 0.503 -2.168 -1.273 -8.367
Hunt & Reffert (2023) 191.018 -58.092 0.529 -2.214 -1.269 -5.05
Cavallo et al. (2024) 191.017 -58.095 0.529
Hunt & Reffert (2024) 191.018 -58.092 0.529 -2.214 -1.269 -5.05
Almeida et al. (2025) 190.997 -58.093
Hu & Soubiran (2025) 191.017 -58.095
           
UCC 191.022 -58.095 0.527 -2.199 -1.249 -8.805
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Liu & Pang (2019) Age=0.832, Z=0.25
Cantat-Gaudin et al. (2020) AVNN=1.22, DistPc=1905.0, AgeNN=8.86
Dias et al. (2021) Av=1.529, Dist=1927, logage=8.818, [Fe/H]=-0.027
Hunt & Reffert (2023) AV50=1.195, diffAV50=1.513, MOD50=11.24, logAge50=8.711
Cavallo et al. (2024) AV50=1.07, dMod50=11.21, logAge50=8.98, [Fe/H]50=0.46
Hunt & Reffert (2024) MassJ=1288.55, MassTot=1360.74
Almeida et al. (2025) AV=1.529, Dist=1927, logAge=8.818, MassRk=960.5
Hu & Soubiran (2025) MA22=-0.19, MA23f=-0.24, MA23g=-0.09, MZ23=-0.43, MK24=-0.18, MF24=-0.24

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 288 100.0 191.01 -58.1 0.53 -2.21 -1.26 -8.79 0.2
CWWDL 3107 63.9 191.0 -58.09 0.53 -2.2 -1.25 -8.94 0.0