HSC 1808

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0.35 UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1808 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 107.528 -15.676 0.764 -3.235 1.606 37.736
Hunt & Reffert 2024 107.535 -15.687 0.766 -3.232 1.596 40.061
Cavallo et al. 2024 107.538 -15.667 0.765 – – –
Hunt & Reffert 2023 107.535 -15.687 0.766 -3.232 1.596 40.061

💡 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 – – – – – 121* – –
Cavallo et al. 2024 1.26 0.72 – 15 -0.450 – – –
Hunt & Reffert 2023 1.21 0.44 1.06 31 – – – –

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

Visualization

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