OC 0508

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0.54 UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0508 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 137.546 -49.79 0.399 -5.586 5.602 –
Hunt & Reffert 2024 137.546 -49.793 0.385 -5.567 5.578 –
Cavallo et al. 2024 137.576 -49.833 0.386 – – –
Hunt & Reffert 2023 137.546 -49.793 0.385 -5.567 5.578 –
Hao et al. 2022 137.506 -49.801 0.401 -5.594 5.517 –

💡 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 – – – – – 756* – –
Cavallo et al. 2024 2.50 4.66 – 47 0.420 – – –
Hunt & Reffert 2023 2.32 4.36 2.74 17 – – – –
Hao et al. 2022 – 1.25 – 1 0.274 – – –

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

Visualization

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