HSC 1852

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0.28 UTI
0.41
CN
0.49
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1852 is a poorly populated, loose object of intermediate 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, young cluster (see Parameters). It was recently reported in the literature.
Distant 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 – 112.615 -19.017 0.292 -2.256 2.97 129.139
Hunt & Reffert 2024 112.597 -19.008 0.285 -2.19 2.943 129.232
Cavallo et al. 2024 112.623 -19.009 0.291 – – –
Hunt & Reffert 2023 112.597 -19.008 0.285 -2.19 2.943 129.232

💡 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 – – – – – 274* – –
Cavallo et al. 2024 3.09 1.58 – 47 0.420 – – –
Hunt & Reffert 2023 2.93 1.87 1.98 32 – – – –

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

Visualization

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