OC 0315

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0.51 UTI
0.31
CN
1.0
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0315 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 94.923 22.119 0.543 0.634 -2.529 25.812
Zhang et al. 2024 94.936 22.115 – – – –
Hunt & Reffert 2024 94.936 22.115 0.547 0.624 -2.502 22.537
Cavallo et al. 2024 94.912 22.17 0.546 – – –
Hunt & Reffert 2023 94.936 22.115 0.547 0.624 -2.502 22.537
Hao et al. 2022 94.924 22.1 0.542 0.577 -2.55 –

💡 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 – – – – -0.296* – – –
Hunt & Reffert 2024 – – – – – 296* – –
Cavallo et al. 2024 1.74 1.55 – 6 -0.150 – – –
Hunt & Reffert 2023 1.70 1.66 1.78 10 – – – –
Hao et al. 2022 – 2.71 – 8 0.169 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14033 93.5 94.92 22.11 0.54 0.65 -2.56 25.81 0.07

💡 Note: The % column shows the percentage of members that OC 0315 shares with each listed object.

Visualization

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