HSC 917

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0.21 UTI
0.0
CN
0.56
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.56 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 917 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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 High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 354.647 63.489 0.219 -2.36 -0.966 -77.79
Hunt & Reffert 2024 354.638 63.491 0.236 -2.337 -0.972 -77.728
Cavallo et al. 2024 354.722 63.49 0.239 – – –
Hunt & Reffert 2023 354.638 63.491 0.236 -2.337 -0.972 -77.728

💡 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 – – – – – 351* – –
Cavallo et al. 2024 3.93 3.67 – 251 -0.150 – – –
Hunt & Reffert 2023 3.52 3.44 1.83 379 – – – –

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

Visualization

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