OC 0403

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0.43 UTI
0.25
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0403 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity 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 – 113.311 -20.162 0.339 -2.285 3.306 80.557
Hunt & Reffert 2024 113.309 -20.16 0.35 -2.273 3.284 –
Cavallo et al. 2024 113.315 -20.16 0.346 – – –
Hunt & Reffert 2023 113.309 -20.16 0.35 -2.273 3.284 –
Hao et al. 2022 113.326 -20.155 0.334 -2.25 3.289 –

💡 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 – – – – – 450* – –
Cavallo et al. 2024 2.42 1.67 – 32 -0.050 – – –
Hunt & Reffert 2023 2.74 1.57 1.17 56 – – – –
Hao et al. 2022 – 0.70 – 8 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 321 100.0 113.31 -20.16 0.35 -2.3 3.31 80.56 0.24
CWWDL 6375 4.0 113.54 -20.22 0.33 -2.13 3.25 56.66 0.03

💡 Note: The % column shows the percentage of members that OC 0403 shares with each listed object.

Visualization

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