OC 0465

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0.25 UTI
0.35
CN
0.17
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0465 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.42 kpc) differs significantly from the median photometric distance (~4.62 kpc).

Distant High extinction Massive Near-solar metallicity 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 – 127.313 -41.199 0.156 -2.777 3.548 –
Hunt & Reffert 2024 127.314 -41.219 0.166 -2.787 3.57 78.22
Cavallo et al. 2024 127.258 -41.203 0.164 – – –
Hunt & Reffert 2023 127.314 -41.219 0.166 -2.787 3.57 78.22
Hao et al. 2022 127.332 -41.189 0.151 -2.755 3.559 –

💡 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 – – – – – 1470* – –
Cavallo et al. 2024 3.98 3.05 – 209 0.000 – – –
Hunt & Reffert 2023 5.25 3.15 2.53 32 – – – –
Hao et al. 2022 – 3.62 – 5 0.611 – – –

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

Visualization

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