UBC 1157

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0.21 UTI
0.49
CN
0.46
Cdens
0.75
CC3
0.31
Clit
0.45
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 0.46 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 0.45 Possibly duplicate

Overview

â„šī¸
UBC 1157 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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.

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.

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 – 335.686 53.731 0.301 -2.833 -2.463 -60.916
Hu & Soubiran 2025 335.635 53.723 – – – –
Hunt & Reffert 2024 335.699 53.724 0.294 -2.831 -2.454 -60.854
Cavallo et al. 2024 335.635 53.723 0.298 – – –
Hunt & Reffert 2023 335.699 53.724 0.294 -2.831 -2.454 -60.854
Castro-Ginard et al. 2022 335.67 53.73 0.31 -2.84 -2.45 –

💡 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
Hu & Soubiran 2025 – – – – -0.210* – – –
Hunt & Reffert 2024 – – – – – 340* – –
Cavallo et al. 2024 2.45 1.49 – 562 -0.500 – – –
Hunt & Reffert 2023 3.26 0.83 1.19 489 – – – –
Castro-Ginard et al. 2022 3.46 0.82 – 166 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 574 95.9 335.69 53.73 0.3 -2.84 -2.46 -60.92 0.05
LISC 1103 55.1 335.68 53.71 0.3 -2.85 -2.48 -58.26 0.43

💡 Note: The % column shows the percentage of members that UBC 1157 shares with each listed object.

Visualization

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