HSC 2779

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0.44 UTI
0.27
CN
0.93
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.93 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2779 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Metal-rich Intermediate age

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 – 245.42 -47.265 0.338 -1.339 -1.786 -13.041
Hunt & Reffert 2024 245.421 -47.268 0.341 -1.393 -1.823 -7.167
Cavallo et al. 2024 245.424 -47.286 0.336 – – –
Hunt & Reffert 2023 245.421 -47.268 0.341 -1.393 -1.823 -7.167

💡 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 – – – – – 519* – –
Cavallo et al. 2024 2.41 3.84 – 182 0.580 – – –
Hunt & Reffert 2023 2.71 3.80 2.04 316 – – – –

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

Visualization

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