HSC 1012

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0.36 UTI
0.31
CN
0.76
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.76 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1012 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 – 20.144 63.336 0.306 -3.257 0.456 -71.762
Hunt & Reffert 2024 20.166 63.339 0.309 -3.222 0.457 -71.742
Cavallo et al. 2024 20.129 63.317 0.306 – – –
Hunt & Reffert 2023 20.166 63.339 0.309 -3.222 0.457 -71.742

💡 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 – – – – – 379* – –
Cavallo et al. 2024 4.19 3.90 – 120 0.150 – – –
Hunt & Reffert 2023 2.92 3.68 1.77 290 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3042 83.9 20.14 63.33 0.31 -3.27 0.46 -71.76 0.06

💡 Note: The % column shows the percentage of members that HSC 1012 shares with each listed object.

Visualization

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