UBC 1018

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0.67 UTI
0.87
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.87 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1018 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Very massive Near-solar metallicity Young

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 – 275.916 -12.912 0.361 -0.104 -0.726 18.307
Hunt & Reffert 2024 275.913 -12.918 0.376 -0.121 -0.739 63.893
Cavallo et al. 2024 275.915 -12.891 0.371 – – –
Hunt & Reffert 2023 275.913 -12.918 0.376 -0.121 -0.739 63.893
Castro-Ginard et al. 2022 275.9 -12.91 0.37 -0.12 -0.71 17.6

💡 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 – – – – – 7309* – –
Cavallo et al. 2024 1.83 5.36 – 65 -0.340 – – –
Hunt & Reffert 2023 2.34 4.96 3.07 48 – – – –
Castro-Ginard et al. 2022 2.73 4.09 – 299 – – – –

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

Visualization

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