UBC 313

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0.09 UTI
0.0
CN
0.85
Cdens
1.0
CC3
0.0
Clit
0.24
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.85 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.24 Likely duplicate

Overview

â„šī¸
UBC 313 is a sparse, dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Castro-Ginard et al. (2020)
Tentative identification with Kharchenko et al. (2013, Cat. J/A+A/558/A53), see Sect. 4.1.3.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 246.111 -51.924 0.321 -3.147 -4.343 –
Li et al. 2025 246.139 -51.932 0.3 -3.093 -4.325 –
Cantat-Gaudin et al. 2020 246.139 -51.932 0.3 -3.093 -4.325 –
Castro-Ginard et al. 2020 246.153 -51.938 0.296 -3.075 -4.31 –

💡 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
Li et al. 2025 2.16 1.09 – 518 -0.088 – – –
Cantat-Gaudin et al. 2020 3.24 1.25 – 60 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ruprecht 118 76.0 246.11 -51.92 0.34 -3.17 -4.34 -58.54 0.71

💡 Note: The % column shows the percentage of members that UBC 313 shares with each listed object.

Visualization

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