HSC 903

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0.09 UTI
0.0
CN
0.19
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 903 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Palma et al. (2025)
Part of multiple system G200, along with HSC_907 and UBC_1185.

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 99999– 351.701 62.075 0.329 -3.701 -1.871 -60.255
Hunt & Reffert 2024 351.738 62.07 0.324 -3.694 -1.893 –
Cavallo et al. 2024 351.687 62.074 0.326 – – –
Hunt & Reffert 2023 351.738 62.07 0.324 -3.694 -1.893 –

💡 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] Bfrac BSS
UCC 99999– 2.57 2.94 1.65 48 0.210 239 – –
Hunt & Reffert 2024 – – – – – 239(1) – –
Cavallo et al. 2024 2.30 2.86 – 21 0.210 – – –
Hunt & Reffert 2023 2.84 3.02 1.65 74 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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