OC 0243

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0.25 UTI
0.32
CN
0.37
Cdens
0.75
CC3
0.25
Clit
0.66
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.37 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.66 Likely unique

Overview

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OC 0243 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate 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 is likely a unique object, which shares a moderate percentage of members with at least one previously 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 – 37.356 62.958 0.316 -0.304 -0.192 –
Hunt & Reffert 2024 37.281 62.949 0.319 -0.318 -0.151 –
Cavallo et al. 2024 37.292 62.951 0.317 – – –
Hunt & Reffert 2023 37.281 62.949 0.319 -0.318 -0.151 –
Hao et al. 2022 37.333 62.985 0.316 -0.283 -0.238 –

💡 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
Hunt & Reffert 2024 – – – – – 241* – –
Cavallo et al. 2024 2.90 2.14 – 11 0.260 – – –
Hunt & Reffert 2023 2.82 2.02 1.89 28 – – – –
Hao et al. 2022 – 2.06 – 13 0.370 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1925 34.4 37.47 62.97 0.28 -0.3 -0.14 -34.67 0.04

💡 Note: The % column shows the percentage of members that OC 0243 shares with each listed object.

Visualization

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