HSC 1036

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0.22 UTI
0.28
CN
0.34
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1036 is a poorly populated, 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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.

Distant 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 – 25.132 60.934 0.214 -1.536 -0.747 –
Hunt & Reffert 2024 25.15 60.908 0.221 -1.523 -0.744 -10.235
Cavallo et al. 2024 25.1 60.938 0.22 – – –
Hunt & Reffert 2023 25.15 60.908 0.221 -1.523 -0.744 -10.235

💡 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 – – – – – 335* – –
Cavallo et al. 2024 3.42 1.95 – 355 0.140 – – –
Hunt & Reffert 2023 4.08 2.06 1.47 204 – – – –

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

Visualization

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