HSC 436

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0.49 UTI
0.69
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.69 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 436 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very 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 object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Very 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 – 291.313 18.723 0.184 -2.528 -3.562 42.91
Hunt & Reffert 2024 291.309 18.725 0.191 -2.53 -3.569 42.936
Cavallo et al. 2024 291.305 18.728 0.186 – – –
Hunt & Reffert 2023 291.309 18.725 0.191 -2.53 -3.569 42.936

💡 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 – – – – – 3926* – –
Cavallo et al. 2024 4.72 4.78 – 407 0.370 – – –
Hunt & Reffert 2023 4.41 5.32 2.30 748 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3632 100.0 291.31 18.72 0.19 -2.54 -3.57 42.91 0.2

💡 Note: The % column shows the percentage of members that HSC 436 shares with each listed object.

Visualization

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