OC 0037

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0.48 UTI
0.29
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0037 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Massive Metal-rich 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 – 278.105 -10.584 0.491 0.59 -0.214 31.982
Hunt & Reffert 2024 278.09 -10.594 0.489 0.592 -0.201 80.907
Cavallo et al. 2024 278.089 -10.593 0.489 – – –
Hunt & Reffert 2023 278.09 -10.594 0.489 0.592 -0.201 80.907
Hao et al. 2022 278.09 -10.57 0.522 0.646 -0.205 -10.361

💡 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 – – – – – 1103* – –
Cavallo et al. 2024 1.97 4.40 – 85 0.930 – – –
Hunt & Reffert 2023 1.92 4.95 2.53 36 – – – –
Hao et al. 2022 – 4.85 – 50 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 43 48.3 278.09 -10.59 0.49 0.53 -0.17 167.41 0.13

💡 Note: The % column shows the percentage of members that OC 0037 shares with each listed object.

Visualization

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