HSC 1759

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0.28 UTI
0.25
CN
0.4
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.4 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1759 is a poorly populated, 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
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 – 107.43 -9.605 0.329 -0.748 -0.264 –
Hunt & Reffert 2024 107.428 -9.606 0.333 -0.763 -0.261 –
Cavallo et al. 2024 107.434 -9.595 0.333 – – –
Hunt & Reffert 2023 107.428 -9.606 0.333 -0.763 -0.261 –

💡 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 – – – – – 224* – –
Cavallo et al. 2024 2.81 1.25 – 468 0.180 – – –
Hunt & Reffert 2023 2.90 1.13 0.30 182 – – – –

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

Visualization

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