HSC 1532

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0.24 UTI
0.0
CN
0.07
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1532 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 95.375 18.05 0.284 -0.027 -1.096 –
Zhang et al. 2024 95.417 18.069 – – – –
Hunt & Reffert 2024 95.417 18.069 0.275 0.018 -1.114 55.779
Cavallo et al. 2024 95.45 18.029 0.275 – – –
Hunt & Reffert 2023 95.417 18.069 0.275 0.018 -1.114 55.779

💡 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
Zhang et al. 2024 – – – – -0.181* – – –
Hunt & Reffert 2024 – – – – – 338* – –
Cavallo et al. 2024 2.83 1.35 – 380 -0.170 – – –
Hunt & Reffert 2023 3.10 1.25 1.67 210 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3202 72.0 95.43 18.02 0.28 -0.06 -1.08 – 0.07

💡 Note: The % column shows the percentage of members that HSC 1532 shares with each listed object.

Visualization

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