HSC 1028

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0.06 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1028 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above 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 significant 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.

Very distant Moderate extinction Near-solar metallicity Young

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 – 25.287 64.272 0.168 -1.458 -0.109 –
Hunt & Reffert 2024 25.301 64.276 0.167 -1.425 -0.096 -49.319
Cavallo et al. 2024 25.428 64.25 0.168 – – –
Hunt & Reffert 2023 25.301 64.276 0.167 -1.425 -0.096 -49.319

💡 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 – – – – – 562* – –
Cavallo et al. 2024 5.75 2.63 – 32 0.290 – – –
Hunt & Reffert 2023 4.99 2.62 2.36 48 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4144 68.0 25.47 64.27 0.18 -1.46 -0.08 -82.43 0.04

💡 Note: The % column shows the percentage of members that HSC 1028 shares with each listed object.

Visualization

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