UBC 1305

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0.38 UTI
0.34
CN
0.79
Cdens
0.38
CC3
0.31
Clit
0.88
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.79 Dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 0.88 Very likely unique

Overview

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UBC 1305 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a relatively close distance, above 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 is very likely a unique object, which shares a small 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 93.939 22.623 0.517 -0.352 -1.666 –
Zhang et al. 2024 93.939 22.588 – – – –
Hunt & Reffert 2024 93.939 22.588 0.519 -0.358 -1.66 –
Cavallo et al. 2024 93.914 22.611 0.519 – – –
Hunt & Reffert 2023 93.939 22.588 0.519 -0.358 -1.66 –
Castro-Ginard et al. 2022 93.92 22.61 0.51 -0.34 -1.66 –

💡 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
Zhang et al. 2024 – – – – -0.278* – – –
Hunt & Reffert 2024 – – – – – 215* – –
Cavallo et al. 2024 2.00 2.38 – 52 -0.060 – – –
Hunt & Reffert 2023 1.82 1.97 1.35 20 – – – –
Castro-Ginard et al. 2022 2.21 1.59 – 72 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10843 100.0 93.93 22.62 0.52 -0.36 -1.66 – 0.03
Teutsch 170 11.8 93.85 22.85 0.45 -0.31 -1.61 – 0.07

💡 Note: The % column shows the percentage of members that UBC 1305 shares with each listed object.

Visualization

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