HSC 516

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0.36 UTI
0.25
CN
0.29
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 516 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
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 – 299.731 27.154 1.048 0.43 -2.203 -14.7
Zhang et al. 2024 299.745 27.196 – – – –
Hunt & Reffert 2024 299.745 27.196 1.05 0.43 -2.238 -11.737
Cavallo et al. 2024 299.659 26.945 1.043 – – –
Hunt & Reffert 2023 299.745 27.196 1.05 0.43 -2.238 -11.737

💡 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 – – – – -0.239* – – –
Hunt & Reffert 2024 – – – – – 77* – –
Cavallo et al. 2024 0.96 0.81 – 224 0.490 – – –
Hunt & Reffert 2023 0.92 0.97 1.04 97 – – – –

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

Visualization

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