UBC 1562

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0.30 UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.47
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.66 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.47 Possibly duplicate

Overview

â„šī¸
UBC 1562 is a moderately 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, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously 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 – 256.466 -43.462 0.417 -0.919 -3.556 -14.182
Hunt & Reffert 2024 256.484 -43.455 0.417 -0.906 -3.514 17.606
Cavallo et al. 2024 256.444 -43.472 0.415 – – –
Hunt & Reffert 2023 256.484 -43.455 0.417 -0.906 -3.514 17.606
Castro-Ginard et al. 2022 256.45 -43.46 0.41 -0.92 -3.54 -25.83

💡 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 – – – – – 1167* – –
Cavallo et al. 2024 2.10 4.33 – 186 0.070 – – –
Hunt & Reffert 2023 2.23 4.27 2.56 134 – – – –
Castro-Ginard et al. 2022 2.70 3.36 – 121 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 090 53.1 256.49 -43.44 0.41 -0.92 -3.55 6.97 0.5

💡 Note: The % column shows the percentage of members that UBC 1562 shares with each listed object.

Visualization

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