HSC 1003

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0.27 UTI
0.45
CN
0.17
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1003 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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 99999– 19.152 64.818 0.138 -1.458 0.09 -102.315
Hunt & Reffert 2024 19.168 64.84 0.145 -1.429 0.076 -102.297
Cavallo et al. 2024 19.142 64.807 0.145 – – –
Hunt & Reffert 2023 19.168 64.84 0.145 -1.429 0.076 -102.297

💡 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– 6.52 3.25 2.67 16 0.060 1156 – –
Hunt & Reffert 2024 – – – – – 1156(1) – –
Cavallo et al. 2024 6.98 3.21 – 17 0.060 – – –
Hunt & Reffert 2023 6.06 3.29 2.67 15 – – – –

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

Visualization

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