HSC 622

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0.25 UTI
0.32
CN
0.16
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 17.0 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 622 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 307.929 40.716 0.778 -0.16 -3.255 -2.849
Zhang et al. 2024 307.863 40.732 – – – –
Hunt & Reffert 2024 307.863 40.732 0.762 -0.095 -3.248 -15.627
Cavallo et al. 2024 308.157 40.789 0.763 – – –
Hunt & Reffert 2023 307.863 40.732 0.762 -0.095 -3.248 -15.627

💡 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 – – – – -0.389* – – –
Hunt & Reffert 2024 – – – – – 112* – –
Cavallo et al. 2024 1.45 3.10 – 18 0.160 – – –
Hunt & Reffert 2023 1.23 2.55 2.63 11 – – – –

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

Visualization

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