HSC 657

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0.29 UTI
0.41
CN
0.68
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.68 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 657 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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 – 306.687 46.814 0.377 -2.027 -4.715 -22.156
Hunt & Reffert 2024 306.688 46.825 0.36 -2.034 -4.7 -22.166
Cavallo et al. 2024 306.742 46.786 0.359 – – –
Hunt & Reffert 2023 306.688 46.825 0.36 -2.034 -4.7 -22.166

💡 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 – – – – – 178* – –
Cavallo et al. 2024 2.47 2.93 – 39 0.230 – – –
Hunt & Reffert 2023 2.59 2.67 2.04 84 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3250 56.1 306.69 46.82 0.38 -2.01 -4.71 -8.61 0.02

💡 Note: The % column shows the percentage of members that HSC 657 shares with each listed object.

Visualization

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