HSC 1767

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0.40 UTI
0.35
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1767 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 moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Very 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 – 107.295 -10.71 0.82 -3.756 1.075 15.937
Hunt & Reffert 2024 107.268 -10.693 0.846 -3.759 1.075 18.571
Cavallo et al. 2024 107.296 -10.687 0.844 – – –
Hunt & Reffert 2023 107.268 -10.693 0.846 -3.759 1.075 18.571

💡 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 – – – – – 136* – –
Cavallo et al. 2024 1.21 1.51 – 4 -0.350 – – –
Hunt & Reffert 2023 1.15 1.05 1.47 8 – – – –

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

Visualization

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