HSC 438

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0.36 UTI
0.45
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.45 Poorly 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 438 is a poorly populated, very dense object of low 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.

Very distant Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 290.491 19.252 0.184 -1.292 -4.676 0.757
Hunt & Reffert 2024 290.488 19.269 0.169 -1.279 -4.663 30.158
Cavallo et al. 2024 290.485 19.266 0.169 – – –
Hunt & Reffert 2023 290.488 19.269 0.169 -1.279 -4.663 30.158

💡 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 – – – – – 2355* – –
Cavallo et al. 2024 5.89 5.21 – 195 0.160 – – –
Hunt & Reffert 2023 4.53 5.36 2.21 581 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3412 100.0 290.49 19.26 0.18 -1.3 -4.7 0.76 0.1

💡 Note: The % column shows the percentage of members that HSC 438 shares with each listed object.

Visualization

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