HSC 2358

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0.22 UTI
0.0
CN
0.49
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.49 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2358 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a 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.

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 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 – 160.504 -58.439 0.382 -7.16 2.949 –
Hunt & Reffert 2024 160.409 -58.469 0.38 -7.161 2.956 –
Cavallo et al. 2024 160.5 -58.436 0.38 – – –
Hunt & Reffert 2023 160.409 -58.469 0.38 -7.161 2.956 –

💡 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 – – – – – 209* – –
Cavallo et al. 2024 2.51 1.33 – 22 0.200 – – –
Hunt & Reffert 2023 2.62 1.46 1.47 30 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3641 96.0 160.52 -58.44 0.39 -7.17 2.95 -97.61 0.11

💡 Note: The % column shows the percentage of members that HSC 2358 shares with each listed object.

Visualization

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