HSC 2620

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0.35 UTI
0.44
CN
0.56
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 0.56 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2620 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High 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 – 210.297 -63.671 0.279 -7.932 -2.269 -38.79
Hunt & Reffert 2024 210.277 -63.676 0.283 -7.914 -2.258 -51.604
Cavallo et al. 2024 210.3 -63.677 0.283 – – –
Hunt & Reffert 2023 210.277 -63.676 0.283 -7.914 -2.258 -51.604

💡 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 – – – – – 551* – –
Cavallo et al. 2024 2.40 3.06 – 437 -0.130 – – –
Hunt & Reffert 2023 3.19 3.02 2.07 182 – – – –

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

Visualization

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