HSC 554

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0.54 UTI
0.7
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.7 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 554 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young 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 Massive Near-solar metallicity Young

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 – 300.228 32.962 0.24 -2.567 -4.779 1.393
Hunt & Reffert 2024 300.24 32.945 0.24 -2.569 -4.781 -24.867
Cavallo et al. 2024 300.226 32.971 0.24 – – –
Hunt & Reffert 2023 300.24 32.945 0.24 -2.569 -4.781 -24.867

💡 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 – – – – – 1385* – –
Cavallo et al. 2024 3.30 2.52 – 32 0.120 – – –
Hunt & Reffert 2023 3.85 2.50 2.51 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3211 100.0 300.23 32.96 0.24 -2.56 -4.78 -12.87 0.11

💡 Note: The % column shows the percentage of members that HSC 554 shares with each listed object.

Visualization

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