UBC 481

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0.18 UTI
0.75
CN
0.75
Cdens
0.75
CC3
0.25
Clit
0.32
Cdup
Radius (P>50% members) 12.2 [arcmin]
  • CN 0.75 Rich
  • Cdens 0.75 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.32 Possibly duplicate

Overview

â„šī¸
UBC 481 is a rich, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 130.881 -45.808 0.657 -5.028 4.643 13.238
Hunt & Reffert 2024 130.886 -45.852 0.657 -5.021 4.646 20.351
Cavallo et al. 2024 130.901 -45.784 0.658 – – –
Hunt & Reffert 2023 130.886 -45.852 0.657 -5.021 4.646 20.351
Castro-Ginard et al. 2020 130.845 -45.771 0.65 -5.066 4.642 –

💡 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 – – – – – 505* – –
Cavallo et al. 2024 1.50 1.37 – 20 -0.020 – – –
Hunt & Reffert 2023 1.44 1.23 2.21 48 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2219 67.9 130.87 -45.8 0.66 -5.04 4.62 6.12 0.55

💡 Note: The % column shows the percentage of members that UBC 481 shares with each listed object.

Visualization

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