FoF 58

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0.14 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.25
Cdup
Radius (P>50% members) 6.2 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.25 Possibly duplicate

Overview

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FoF 58 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

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.

Near-solar metallicity Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 129.902 -46.287 0.54 -5.833 5.087 -1.51
Liu & Pang 2019 129.957 -46.364 0.524 -5.813 5.063 –

💡 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
Liu & Pang 2019 – – – 23 0.250 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Pismis 6 75.2 129.83 -46.25 0.54 -5.87 5.11 17.73 0.96
OC 0481 18.2 129.65 -46.22 0.54 -5.81 5.15 -9.58 0.19
OC 0484 10.2 130.25 -46.52 0.54 -5.74 5.05 41.74 0.11
CWWDL 13332 9.5 129.66 -46.26 0.54 -5.78 5.13 -9.58 0.01
Pismis 8 6.6 130.39 -46.27 0.54 -5.71 4.99 – 0.95
OC 0482 4.4 130.27 -46.41 0.56 -5.79 5.1 – 0.13
OC 0485 4.4 130.17 -46.65 0.55 -5.7 5.01 – 0.13

💡 Note: The % column shows the percentage of members that FoF 58 shares with each listed object.

Visualization

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