HSC 1622

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0.20 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 16.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1622 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction Low mass 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 – 99.547 6.136 0.761 0.252 -3.678 20.908
Zhang et al. 2024 99.567 6.161 – – – –
Hunt & Reffert 2024 99.567 6.161 0.76 0.261 -3.666 31.753
Cavallo et al. 2024 99.526 6.116 0.76 – – –
Hunt & Reffert 2023 99.567 6.161 0.76 0.261 -3.666 31.753

💡 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 – – – – -0.162* – – –
Hunt & Reffert 2024 – – – – – 45* – –
Cavallo et al. 2024 1.31 0.73 – 224 0.290 – – –
Hunt & Reffert 2023 1.21 0.65 0.80 159 – – – –

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

Visualization

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