HSC 873

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0.19 UTI
0.0
CN
0.3
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 37.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 873 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young 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.

Very close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 345.189 62.288 2.753 7.396 -2.455 -15.169
Cavallo et al. 2024 345.386 62.217 2.739 – – –
Hunt & Reffert 2023 345.063 61.997 2.743 7.402 -2.455 -30.651

💡 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
Cavallo et al. 2024 0.38 1.24 – 15 0.410 – – –
Hunt & Reffert 2023 0.36 0.96 1.31 22 – – – –

Visualization

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