HSC 2649

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0.37 UTI
0.25
CN
0.84
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.84 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2649 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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.
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 – 217.999 -61.953 0.417 -5.207 -3.285 -33.691
Hunt & Reffert 2024 217.986 -61.945 0.406 -5.202 -3.283 -33.681
Cavallo et al. 2024 218.004 -61.949 0.409 – – –
Hunt & Reffert 2023 217.986 -61.945 0.406 -5.202 -3.283 -33.681

💡 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 – – – – – 203* – –
Cavallo et al. 2024 2.04 2.28 – 31 -0.440 – – –
Hunt & Reffert 2023 2.29 1.83 1.53 38 – – – –

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

Visualization

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