OC 0673

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0.55 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0673 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close 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.
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 – 252.623 -41.598 0.614 -0.919 -2.004 -31.488
Hunt & Reffert 2024 252.618 -41.601 0.612 -0.906 -2.011 -34.279
Cavallo et al. 2024 252.642 -41.602 0.612 – – –
Hunt & Reffert 2023 252.618 -41.601 0.612 -0.906 -2.011 -34.279
Hao et al. 2022 252.621 -41.595 0.613 -0.933 -2.036 –

💡 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 – – – – – 198* – –
Cavallo et al. 2024 1.43 0.71 – 11 0.260 – – –
Hunt & Reffert 2023 1.56 1.38 0.76 7 – – – –
Hao et al. 2022 – 3.55 – 6 0.611 – – –

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

Visualization

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