HSC 2769

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0.25 UTI
0.28
CN
0.35
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 16.8 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.35 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2769 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close 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.
Close Moderate extinction Near-solar metallicity Young

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 – 242.383 -47.023 1.224 -0.281 -5.749 -18.521
Hunt & Reffert 2024 242.629 -47.295 1.241 -0.404 -5.773 -12.727
Cavallo et al. 2024 242.404 -46.961 1.231 – – –
Hunt & Reffert 2023 242.629 -47.295 1.241 -0.404 -5.773 -12.727

💡 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 – – – – – 52* – –
Cavallo et al. 2024 0.81 1.27 – 30 0.230 – – –
Hunt & Reffert 2023 0.77 1.29 1.69 19 – – – –

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

Visualization

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