UBC 1290

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0.45 UTI
0.48
CN
0.38
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1290 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a 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.

Distant Moderate extinction 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 – 87.545 30.394 0.296 0.066 -1.371 12.296
Zhang et al. 2024 87.561 30.398 – – – –
Hunt & Reffert 2024 87.561 30.398 0.295 0.067 -1.369 12.328
Cavallo et al. 2024 87.52 30.387 0.295 – – –
Hunt & Reffert 2023 87.561 30.398 0.295 0.067 -1.369 12.328
Castro-Ginard et al. 2022 87.53 30.39 0.31 0.07 -1.37 –

💡 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
Zhang et al. 2024 – – – – 0.115* – – –
Hunt & Reffert 2024 – – – – – 350* – –
Cavallo et al. 2024 3.36 1.25 – 132 0.400 – – –
Hunt & Reffert 2023 3.07 1.03 1.29 213 – – – –
Castro-Ginard et al. 2022 3.99 0.97 – 73 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 146 87.5 87.53 30.41 0.29 0.07 -1.38 12.3 0.03

💡 Note: The % column shows the percentage of members that UBC 1290 shares with each listed object.

Visualization

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