HSC 2819

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0.41 UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.4 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2819 is a poorly populated, very dense object of high 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity 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 – 251.348 -45.834 0.938 -1.758 -5.351 -31.116
Hunt & Reffert 2024 251.347 -45.817 0.93 -1.786 -5.385 -31.811
Cavallo et al. 2024 251.312 -45.883 0.932 – – –
Hunt & Reffert 2023 251.347 -45.817 0.93 -1.786 -5.385 -31.811

💡 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 – – – – – 128* – –
Cavallo et al. 2024 1.05 0.71 – 1122 0.370 – – –
Hunt & Reffert 2023 1.01 1.16 1.22 381 – – – –

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

Visualization

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