HSC 936

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0.45 UTI
0.75
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.99
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.99 Unique

Overview

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HSC 936 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 356.829 68.247 0.213 -2.507 -0.064 -75.188
Hunt & Reffert 2024 356.831 68.252 0.221 -2.514 -0.085 -62.74
Cavallo et al. 2024 356.788 68.239 0.207 – – –
Hunt & Reffert 2023 356.831 68.252 0.221 -2.514 -0.085 -62.74

💡 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 – – – – – 1220* – –
Cavallo et al. 2024 3.19 3.28 – 832 -0.070 – – –
Hunt & Reffert 2023 4.16 3.39 2.51 635 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3284 92.3 356.83 68.24 0.22 -2.5 -0.07 -75.19 0.08
CWNU 2851 1.0 357.07 68.27 0.3 -3.03 0.09 -50.76 0.12

💡 Note: The % column shows the percentage of members that HSC 936 shares with each listed object.

Visualization

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