HSC 1657

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0.06 UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.0
Clit
0.6
Cdup
Radius (P>50% members) 12.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.6 Likely unique

Overview

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HSC 1657 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 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.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 101.501 2.525 0.637 -1.283 0.953 54.862
Zhang et al. 2024 101.483 2.516 – – – –
Cavallo et al. 2024 101.535 2.284 0.649 – – –
Hunt & Reffert 2023 101.483 2.516 0.648 -1.256 0.97 54.888

💡 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 – – – – -0.371* – – –
Cavallo et al. 2024 1.56 0.92 – 204 0.320 – – –
Hunt & Reffert 2023 1.47 0.73 0.45 341 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2111 40.0 101.49 2.07 0.64 -1.22 0.95 49.8 0.07

💡 Note: The % column shows the percentage of members that HSC 1657 shares with each listed object.

Visualization

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