HSC 504

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0.24 UTI
0.0
CN
0.96
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.96 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 504 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Near-solar metallicity Very 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 – 298.9 25.018 0.291 -2.633 -6.351 –
Hunt & Reffert 2024 298.897 25.01 0.3 -2.647 -6.331 –
Cavallo et al. 2024 298.891 25.023 0.294 – – –
Hunt & Reffert 2023 298.897 25.01 0.3 -2.647 -6.331 –

💡 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 – – – – – 306* – –
Cavallo et al. 2024 3.58 3.72 – 21 0.480 – – –
Hunt & Reffert 2023 3.14 3.92 1.37 13 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4248 92.0 298.9 25.02 0.29 -2.63 -6.35 – 0.02

💡 Note: The % column shows the percentage of members that HSC 504 shares with each listed object.

Visualization

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