UBC 1057

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0.00 UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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UBC 1057 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 286.721 13.248 0.286 -1.77 -4.978 25.893
Hunt & Reffert 2024 286.722 13.25 0.291 -1.769 -4.974 25.721
Cavallo et al. 2024 286.72 13.25 0.288 – – –
Hunt & Reffert 2023 286.722 13.25 0.291 -1.769 -4.974 25.721
Castro-Ginard et al. 2022 286.72 13.25 0.29 -1.77 -4.98 -17.64

💡 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 – – – – – 2878* – –
Cavallo et al. 2024 3.73 4.32 – 224 -0.030 – – –
Hunt & Reffert 2023 3.09 4.23 2.48 296 – – – –
Castro-Ginard et al. 2022 3.21 3.09 – 678 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0124 100.0 286.72 13.25 0.29 -1.78 -4.98 26.47 0.78
OC 0074 14.5 286.73 13.24 0.28 -1.76 -4.97 25.16 0.0

💡 Note: The % column shows the percentage of members that UBC 1057 shares with each listed object.

Visualization

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