HSC 2657

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0.34 UTI
0.55
CN
0.4
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 16.6 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 0.4 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2657 is a moderately populated, loose object of high 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 221.339 -63.088 0.885 -6.029 -6.421 -30.607
Hunt & Reffert 2024 221.382 -63.088 0.885 -6.028 -6.416 -29.774
Cavallo et al. 2024 221.358 -63.058 0.889 – – –
Hunt & Reffert 2023 221.382 -63.088 0.885 -6.028 -6.416 -29.774

💡 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 – – – – – 143* – –
Cavallo et al. 2024 1.15 1.33 – 132 0.380 – – –
Hunt & Reffert 2023 1.06 1.15 1.75 98 – – – –

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

Visualization

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