HSC 304

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0.52 UTI
0.62
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.62 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 304 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 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.

Relatively close 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 – 280.535 -1.542 0.286 -1.551 -3.664 19.182
Hunt & Reffert 2024 280.533 -1.546 0.285 -1.556 -3.678 20.872
Cavallo et al. 2024 280.542 -1.559 0.288 – – –
Hunt & Reffert 2023 280.533 -1.546 0.285 -1.556 -3.678 20.872

💡 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 – – – – – 1675* – –
Cavallo et al. 2024 2.67 4.59 – 295 -0.070 – – –
Hunt & Reffert 2023 2.96 4.83 2.92 142 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3612 96.0 280.53 -1.54 0.29 -1.55 -3.66 21.38 0.11

💡 Note: The % column shows the percentage of members that HSC 304 shares with each listed object.

Visualization

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