UBC 1077

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0.57 UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1077 is a moderately populated, very dense object of 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, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Massive Near-solar metallicity Intermediate age

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 – 301.023 30.467 0.334 -1.375 -3.605 29.302
Hunt & Reffert 2024 301.015 30.464 0.332 -1.389 -3.608 30.692
Cavallo et al. 2024 301.022 30.482 0.331 – – –
Hunt & Reffert 2023 301.015 30.464 0.332 -1.389 -3.608 30.692
Castro-Ginard et al. 2022 301.03 30.49 0.33 -1.39 -3.62 47.07

💡 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 – – – – – 1349* – –
Cavallo et al. 2024 2.57 4.53 – 316 -0.270 – – –
Hunt & Reffert 2023 2.76 4.29 2.54 237 – – – –
Castro-Ginard et al. 2022 3.08 2.96 – 1054 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1890 92.5 301.02 30.47 0.34 -1.38 -3.61 29.3 0.01

💡 Note: The % column shows the percentage of members that UBC 1077 shares with each listed object.

Visualization

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