HSC 1073

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0.29 UTI
0.25
CN
0.08
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 11.2 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.08 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1073 is a poorly populated, very loose 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.
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 – 30.028 59.173 0.417 -1.382 -0.805 –
Zhang et al. 2024 30.083 59.153 – – – –
Hunt & Reffert 2024 30.083 59.153 0.414 -1.411 -0.83 -9.375
Cavallo et al. 2024 29.87 59.223 0.416 – – –
Hunt & Reffert 2023 30.083 59.153 0.414 -1.411 -0.83 -9.375

💡 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 – – – – 0.113* – – –
Hunt & Reffert 2024 – – – – – 135* – –
Cavallo et al. 2024 2.36 1.55 – 31 0.130 – – –
Hunt & Reffert 2023 2.25 1.66 1.42 26 – – – –

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

Visualization

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