UBC 1564

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0.06 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.11
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.11 Likely duplicate

Overview

â„šī¸
UBC 1564 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 very high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction 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 – 258.944 -38.723 0.259 -1.305 -3.271 -9.572
Cavallo et al. 2024 258.94 -38.729 0.278 – – –
Hunt & Reffert 2023 258.954 -38.721 0.281 -1.307 -3.276 8.458
Castro-Ginard et al. 2022 258.94 -38.72 0.27 -1.31 -3.27 -10.12

💡 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
Cavallo et al. 2024 2.65 5.40 – 44 -0.430 – – –
Hunt & Reffert 2023 3.08 5.21 2.81 47 – – – –
Castro-Ginard et al. 2022 3.63 3.97 – 116 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 86 88.9 258.94 -38.72 0.26 -1.31 -3.27 -9.57 0.55

💡 Note: The % column shows the percentage of members that UBC 1564 shares with each listed object.

Visualization

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