UBC 1028

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0.56 UTI
0.32
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.32 Poorly populated
  • 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 1028 is a poorly populated, 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 massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 278.251 -9.404 0.335 -0.082 -2.024 48.485
Hunt & Reffert 2024 278.252 -9.404 0.341 -0.057 -2.002 117.726
Cavallo et al. 2024 278.247 -9.431 0.339 – – –
Hunt & Reffert 2023 278.252 -9.404 0.341 -0.057 -2.002 117.726
Castro-Ginard et al. 2022 278.25 -9.42 0.34 -0.06 -2.02 –

💡 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 – – – – – 1031* – –
Cavallo et al. 2024 2.44 3.99 – 13 0.200 – – –
Hunt & Reffert 2023 2.65 4.25 2.53 32 – – – –
Castro-Ginard et al. 2022 2.89 3.41 – 66 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1731 75.0 278.24 -9.4 0.34 -0.08 -1.99 183.98 0.02

💡 Note: The % column shows the percentage of members that UBC 1028 shares with each listed object.

Visualization

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