UBC 341

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0.02 UTI
0.72
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.03
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.72 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 0.03 Very likely duplicate

Overview

â„šī¸
UBC 341 is a moderately populated, very 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 massive, near-solar metallicity, very young 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.

Relatively close Moderate extinction Massive Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. 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 – 276.467 -17.074 0.485 -0.222 -1.534 -27.469
Almeida et al. 2025 276.449 -17.077 – – – –
Celli et al. 2024 276.464 -17.076 – – – –
Dias et al. 2021 276.449 -17.077 0.471 -0.195 -1.491 2.32
Cantat-Gaudin et al. 2020 276.464 -17.076 0.478 -0.22 -1.487 –
Castro-Ginard et al. 2020 276.452 -17.063 0.475 -0.208 -1.491 –

💡 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
Almeida et al. 2025 2.04 2.69 – 13 – 1062 – –
Celli et al. 2024 – – – 22 – 993 – –
Dias et al. 2021 2.04 2.69 – 13 0.146 – – –
Cantat-Gaudin et al. 2020 2.00 2.59 – 22 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 265 96.8 276.46 -17.08 0.48 -0.22 -1.56 -27.47 0.65
CWWDL 970 55.3 276.47 -17.07 0.5 -0.24 -1.56 -27.47 0.0

💡 Note: The % column shows the percentage of members that UBC 341 shares with each listed object.

Visualization

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