HSC 2764

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0.34 UTI
0.29
CN
0.65
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2764 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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.

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

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 – 249.577 -52.46 0.661 -1.996 -1.625 -18.499
Hunt & Reffert 2024 249.577 -52.374 0.661 -1.965 -1.632 -19.691
Cavallo et al. 2024 249.531 -52.497 0.662 – – –
Hunt & Reffert 2023 249.577 -52.374 0.661 -1.965 -1.632 -19.691

💡 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 – – – – – 175* – –
Cavallo et al. 2024 1.22 1.65 – 316 -0.110 – – –
Hunt & Reffert 2023 1.43 1.19 0.99 373 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3582 100.0 249.57 -52.46 0.66 -2.0 -1.63 -18.95 0.08

💡 Note: The % column shows the percentage of members that HSC 2764 shares with each listed object.

Visualization

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