HSC 1754

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0.30 UTI
0.48
CN
0.5
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1754 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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.

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 – 105.446 -10.044 0.366 -1.208 0.884 49.735
Hunt & Reffert 2024 105.442 -10.055 0.364 -1.215 0.877 49.742
Cavallo et al. 2024 105.458 -10.038 0.368 – – –
Hunt & Reffert 2023 105.442 -10.055 0.364 -1.215 0.877 49.742

💡 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 – – – – – 254* – –
Cavallo et al. 2024 2.19 1.67 – 30 0.260 – – –
Hunt & Reffert 2023 2.43 1.87 1.85 28 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3526 68.8 105.47 -10.06 0.36 -1.2 0.89 49.73 0.0

💡 Note: The % column shows the percentage of members that HSC 1754 shares with each listed object.

Visualization

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