HSC 1246

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0.16 UTI
0.27
CN
0.17
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1246 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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 High extinction Metal-rich 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 – 68.842 47.126 0.303 -0.404 -0.954 –
Hunt & Reffert 2024 68.961 47.137 0.314 -0.392 -0.958 -14.772
Cavallo et al. 2024 68.827 47.144 0.316 – – –
Hunt & Reffert 2023 68.961 47.137 0.314 -0.392 -0.958 -14.772

💡 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 – – – – – 758* – –
Cavallo et al. 2024 3.94 3.72 – 24 0.500 – – –
Hunt & Reffert 2023 2.77 3.99 2.57 39 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3528 100.0 68.83 47.16 0.3 -0.39 -0.94 -67.28 0.14

💡 Note: The % column shows the percentage of members that HSC 1246 shares with each listed object.

Visualization

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