HSC 925

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0.19 UTI
0.0
CN
0.19
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 15.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 925 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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.

Relatively close Moderate 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 – 354.771 68.537 0.949 -2.375 -2.917 -6.441
Hunt & Reffert 2024 354.77 68.718 0.929 -2.401 -2.945 -8.622
Cavallo et al. 2024 354.155 68.512 0.941 – – –
Hunt & Reffert 2023 354.77 68.718 0.929 -2.401 -2.945 -8.622

💡 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 – – – – – 164* – –
Cavallo et al. 2024 1.22 2.48 – 13 0.350 – – –
Hunt & Reffert 2023 1.01 2.40 2.47 13 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4175 100.0 354.57 68.5 0.95 -2.39 -2.94 -11.41 0.19

💡 Note: The % column shows the percentage of members that HSC 925 shares with each listed object.

Visualization

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