HSC 444

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0.27 UTI
0.27
CN
0.33
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 444 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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 Moderate extinction Metal-rich 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 – 295.097 17.777 0.289 -1.97 -2.554 19.436
Hunt & Reffert 2024 295.127 17.785 0.307 -1.988 -2.568 38.05
Cavallo et al. 2024 295.102 17.793 0.303 – – –
Hunt & Reffert 2023 295.127 17.785 0.307 -1.988 -2.568 38.05

💡 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 – – – – – 397* – –
Cavallo et al. 2024 3.27 2.55 – 170 0.600 – – –
Hunt & Reffert 2023 3.05 2.68 2.27 76 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3408 96.3 295.1 17.78 0.29 -1.98 -2.55 19.44 0.03

💡 Note: The % column shows the percentage of members that HSC 444 shares with each listed object.

Visualization

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