UBC 1070

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0.47 UTI
0.36
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1070 is a poorly populated, very dense object of intermediate 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 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 – 298.409 27.54 0.475 -2.092 -4.53 -5.084
Hunt & Reffert 2024 298.41 27.55 0.474 -2.096 -4.544 -5.092
Cavallo et al. 2024 298.409 27.551 0.474 – – –
Hunt & Reffert 2023 298.41 27.55 0.474 -2.096 -4.544 -5.092
Castro-Ginard et al. 2022 298.41 27.57 0.48 -2.09 -4.52 –

💡 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 – – – – – 326* – –
Cavallo et al. 2024 2.00 2.34 – 22 0.260 – – –
Hunt & Reffert 2023 1.95 2.35 0.88 30 – – – –
Castro-Ginard et al. 2022 2.17 1.92 – 116 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 370 94.4 298.4 27.54 0.48 -2.09 -4.54 -5.08 0.05

💡 Note: The % column shows the percentage of members that UBC 1070 shares with each listed object.

Visualization

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