HSC 1069

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0.38 UTI
0.54
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1069 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant High 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 – 30.271 60.251 0.281 -1.674 -0.386 -62.783
Hunt & Reffert 2024 30.285 60.253 0.291 -1.682 -0.388 -66.37
Cavallo et al. 2024 30.264 60.262 0.289 – – –
Hunt & Reffert 2023 30.285 60.253 0.291 -1.682 -0.388 -66.37

💡 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
Hunt & Reffert 2024 – – – – – 423* – –
Cavallo et al. 2024 3.44 3.51 – 380 0.280 – – –
Hunt & Reffert 2023 3.28 3.18 2.34 393 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3406 100.0 30.27 60.25 0.28 -1.69 -0.39 -62.78 0.15

💡 Note: The % column shows the percentage of members that HSC 1069 shares with each listed object.

Visualization

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