HSC 1472

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0.48 UTI
0.25
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1472 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 86.151 21.861 0.737 0.986 -2.962 14.763
Zhang et al. 2024 86.146 21.847 – – – –
Hunt & Reffert 2024 86.146 21.847 0.733 0.988 -2.959 18.094
Cavallo et al. 2024 86.149 21.863 0.731 – – –
Hunt & Reffert 2023 86.146 21.847 0.733 0.988 -2.959 18.094

💡 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
Zhang et al. 2024 – – – – 0.066* – – –
Hunt & Reffert 2024 – – – – – 89* – –
Cavallo et al. 2024 1.45 0.87 – 1023 -0.020 – – –
Hunt & Reffert 2023 1.31 1.82 1.44 87 – – – –

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

Visualization

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