OC 0357

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0.63 UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0357 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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

Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 91.941 -6.401 1.141 -2.811 1.059 35.997
Zhang et al. 2024 91.932 -6.396 – – – –
Hunt & Reffert 2024 91.932 -6.396 1.125 -2.79 0.99 86.293
Cavallo et al. 2024 91.92 -6.378 1.158 – – –
Hunt & Reffert 2023 91.932 -6.396 1.125 -2.79 0.99 86.293
Hao et al. 2022 91.961 -6.392 1.187 -2.885 1.07 30.584

💡 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
Zhang et al. 2024 – – – – -0.155* – – –
Hunt & Reffert 2024 – – – – – 346* – –
Cavallo et al. 2024 1.02 2.37 – 4 0.030 – – –
Hunt & Reffert 2023 0.82 2.45 2.79 4 – – – –
Hao et al. 2022 – 1.06 – 5 0.575 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2262 94.5 91.95 -6.39 1.14 -2.82 1.06 33.79 0.07

💡 Note: The % column shows the percentage of members that OC 0357 shares with each listed object.

Visualization

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