UPK 447

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0.19 UTI
0.0
CN
0.18
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 17.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UPK 447 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Low mass 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 – 103.987 -10.242 1.007 -3.653 0.459 39.147
Hunt & Reffert 2024 103.906 -10.265 0.99 -3.605 0.415 31.645
Cavallo et al. 2024 104.306 -9.923 0.991 – – –
Hunt & Reffert 2023 103.906 -10.265 0.99 -3.605 0.415 31.645
Sim et al. 2019 104.241 -10.115 – -3.6 0.41 –

💡 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 – – – – – 45* – –
Cavallo et al. 2024 0.98 0.59 – 50 -0.220 – – –
Hunt & Reffert 2023 0.97 0.48 1.09 65 – – – –
Sim et al. 2019 0.96 – – 45 – – – –

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

Visualization

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