OC 0476

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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) 2.3 [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 0476 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Near-solar metallicity Intermediate age

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 – 128.601 -43.832 0.316 -3.016 4.13 30.543
Hunt & Reffert 2024 128.591 -43.837 0.317 -2.993 4.111 30.569
Cavallo et al. 2024 128.603 -43.834 0.318 – – –
Hunt & Reffert 2023 128.591 -43.837 0.317 -2.993 4.111 30.569
Hao et al. 2022 128.603 -43.84 0.324 -3.012 4.103 –

💡 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 – – – – – 885* – –
Cavallo et al. 2024 2.77 4.81 – 380 0.040 – – –
Hunt & Reffert 2023 2.86 4.18 2.62 222 – – – –
Hao et al. 2022 – 2.57 – 794 0.051 – – –

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

Visualization

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