HSC 1025

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0.21 UTI
0.0
CN
0.31
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.31 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1025 is a sparse, loose object of high 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.

Distant 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 – 23.672 61.906 0.316 -1.661 -0.262 –
Hunt & Reffert 2024 23.678 61.894 0.315 -1.673 -0.255 –
Cavallo et al. 2024 23.654 61.903 0.316 – – –
Hunt & Reffert 2023 23.678 61.894 0.315 -1.673 -0.255 –

💡 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 – – – – – 301* – –
Cavallo et al. 2024 3.27 2.60 – 25 -0.010 – – –
Hunt & Reffert 2023 3.01 2.45 0.94 41 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3522 88.0 23.67 61.91 0.31 -1.66 -0.26 – 0.03

💡 Note: The % column shows the percentage of members that HSC 1025 shares with each listed object.

Visualization

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