UBC 1470

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0.36 UTI
0.43
CN
0.1
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.4 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1470 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate 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.

Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Distant 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 – 148.873 -54.14 0.318 -6.162 4.233 –
Hunt & Reffert 2024 148.903 -54.134 0.315 -6.136 4.218 –
Cavallo et al. 2024 148.769 -54.14 0.316 – – –
Hunt & Reffert 2023 148.903 -54.134 0.315 -6.136 4.218 –
Castro-Ginard et al. 2022 148.87 -54.14 0.32 -6.2 4.25 –

💡 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 – – – – – 218* – –
Cavallo et al. 2024 3.03 1.96 – 46 0.260 – – –
Hunt & Reffert 2023 2.82 1.91 2.13 37 – – – –
Castro-Ginard et al. 2022 3.18 1.43 – 67 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1623 27.9 148.56 -53.98 0.31 -6.11 4.22 – 0.12

💡 Note: The % column shows the percentage of members that UBC 1470 shares with each listed object.

Visualization

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