HSC 2470

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0.33 UTI
0.0
CN
0.9
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.9 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2470 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate 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 – 178.866 -61.746 0.408 -5.401 0.085 –
Hunt & Reffert 2024 178.857 -61.745 0.403 -5.399 0.082 –
Cavallo et al. 2024 178.897 -61.736 0.405 – – –
Hunt & Reffert 2023 178.857 -61.745 0.403 -5.399 0.082 –

💡 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 – – – – – 161* – –
Cavallo et al. 2024 1.97 1.23 – 83 -0.410 – – –
Hunt & Reffert 2023 2.33 0.61 0.36 147 – – – –

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

Visualization

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