UBC 19

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0.00 UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members) 14.4 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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UBC 19 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a 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.

Very close Low extinction Near-solar metallicity Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 56.439 29.819 2.471 2.664 -5.227 17.241
Alfonso et al. 2024 56.427 29.891 2.462 2.752 -5.222 –
Celli et al. 2024 56.336 29.827 – – – –
Cantat-Gaudin et al. 2020 56.336 29.827 2.385 2.705 -5.17 –
Cantat-Gaudin & Anders 2020 56.336 29.827 2.385 2.705 -5.17 –
Castro-Ginard et al. 2018 56.484 29.919 2.393 2.72 -5.19 31.38

💡 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
Alfonso et al. 2024 0.42 0.70 – 10 0.088 – – –
Celli et al. 2024 – – – 7 – 143 – –
Cantat-Gaudin et al. 2020 0.42 0.70 – 7 – – – –
Cantat-Gaudin & Anders 2020 0.41 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi Teutsch 10 100.0 56.43 29.82 2.49 2.69 -5.24 18.55 0.72
OCSN 284 96.2 56.45 29.82 2.49 2.68 -5.24 18.55 0.0
OC 0278 57.7 56.37 29.78 2.47 2.57 -5.26 18.05 0.0

💡 Note: The % column shows the percentage of members that UBC 19 shares with each listed object.

Visualization

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