OC 0600

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0.54 UTI
0.46
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.46 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 0600 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, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Near-solar metallicity 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 – 206.968 -63.424 0.325 -6.519 -1.938 -51.801
Hunt & Reffert 2024 206.95 -63.429 0.313 -6.517 -1.965 -34.663
Cavallo et al. 2024 206.998 -63.425 0.317 – – –
Hunt & Reffert 2023 206.95 -63.429 0.313 -6.517 -1.965 -34.663
Hao et al. 2022 206.97 -63.424 0.324 -6.548 -1.947 -51.643

💡 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 – – – – – 923* – –
Cavallo et al. 2024 2.68 3.25 – 55 0.060 – – –
Hunt & Reffert 2023 3.08 3.37 2.93 38 – – – –
Hao et al. 2022 – 0.94 – 25 0.611 – – –

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

Visualization

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