OC 0448

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0.40 UTI
0.36
CN
0.39
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0448 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction 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 – 119.752 -40.13 0.552 -4.139 4.793 –
Hunt & Reffert 2024 119.838 -40.248 0.54 -4.104 4.737 37.785
Cavallo et al. 2024 119.939 -40.194 0.544 – – –
Hunt & Reffert 2023 119.838 -40.248 0.54 -4.104 4.737 37.785
Hao et al. 2022 119.834 -40.179 0.567 -4.187 4.84 –

💡 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 – – – – – 310* – –
Cavallo et al. 2024 1.83 1.52 – 39 0.280 – – –
Hunt & Reffert 2023 1.69 1.34 2.25 155 – – – –
Hao et al. 2022 – 0.02 – 50 0.223 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 150 100.0 119.74 -40.14 0.55 -4.12 4.79 14.4 0.1

💡 Note: The % column shows the percentage of members that OC 0448 shares with each listed object.

Visualization

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