HSC 1001

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0.32 UTI
0.27
CN
0.1
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1001 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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.
Distant Moderate extinction Near-solar metallicity 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 – 17.575 57.73 0.284 -1.069 -0.956 –
Zhang et al. 2024 17.612 57.73 – – – –
Hunt & Reffert 2024 17.612 57.73 0.279 -1.075 -0.928 –
Cavallo et al. 2024 17.585 57.7 0.278 – – –
Hunt & Reffert 2023 17.612 57.73 0.279 -1.075 -0.928 –

💡 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
Zhang et al. 2024 – – – – 0.156* – – –
Hunt & Reffert 2024 – – – – – 203* – –
Cavallo et al. 2024 2.90 1.61 – 16 -0.080 – – –
Hunt & Reffert 2023 3.22 1.55 1.45 37 – – – –

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

Visualization

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