HSC 1753

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0.17 UTI
0.28
CN
0.34
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1753 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low 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 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 Low 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 – 108.292 -8.393 0.378 -1.055 1.02 -14.542
Hunt & Reffert 2024 108.275 -8.329 0.375 -1.071 1.027 -14.547
Cavallo et al. 2024 108.276 -8.384 0.375 – – –
Hunt & Reffert 2023 108.275 -8.329 0.375 -1.071 1.027 -14.547

💡 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 – – – – – 189* – –
Cavallo et al. 2024 2.15 1.00 – 214 0.010 – – –
Hunt & Reffert 2023 2.42 0.69 1.31 150 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3718 100.0 108.29 -8.37 0.38 -1.05 1.02 -14.54 0.05

💡 Note: The % column shows the percentage of members that HSC 1753 shares with each listed object.

Visualization

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