HSC 1235

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0.23 UTI
0.0
CN
0.91
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.91 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1235 is a sparse, very dense object of low 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 – 64.679 45.372 0.33 -0.859 -1.25 –
Hunt & Reffert 2024 64.672 45.365 0.326 -0.852 -1.256 –
Cavallo et al. 2024 64.682 45.379 0.326 – – –
Hunt & Reffert 2023 64.672 45.365 0.326 -0.852 -1.256 –

💡 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 – – – – – 182* – –
Cavallo et al. 2024 2.96 1.97 – 174 0.320 – – –
Hunt & Reffert 2023 3.73 1.91 0.50 162 – – – –

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

Visualization

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