UBC 1356

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0.25 UTI
0.0
CN
0.25
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1356 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Distant Low extinction Near-solar metallicity Intermediate age

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 – 110.461 -6.537 0.247 -1.093 0.826 70.177
Hunt & Reffert 2024 110.459 -6.547 0.233 -1.099 0.825 70.171
Cavallo et al. 2024 110.473 -6.536 0.236 – – –
Hunt & Reffert 2023 110.459 -6.547 0.233 -1.099 0.825 70.171
Castro-Ginard et al. 2022 110.48 -6.51 0.26 -1.09 0.82 69.16

💡 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 – – – – – 404* – –
Cavallo et al. 2024 3.58 0.88 – 372 0.060 – – –
Hunt & Reffert 2023 3.67 0.40 2.10 641 – – – –
Castro-Ginard et al. 2022 3.87 0.46 – 269 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 12017 100.0 110.47 -6.54 0.25 -1.11 0.81 70.18 0.13

💡 Note: The % column shows the percentage of members that UBC 1356 shares with each listed object.

Visualization

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